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Spectroscopic decomposition of NGC 3521: unveiling the properties of the bulge and disc

Lodovico Coccato, Maximilian H Fabricius, Roberto P Saglia, Ralf Bender, Peter Erwin, Niv Drory, Lorenzo Morelli
<span title="2018-03-15">2018</span> <i title="Oxford University Press (OUP)"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/qjdxzupqgjennounydm4zfdlem" style="color: black;">Monthly notices of the Royal Astronomical Society</a> </i> &nbsp;
We study the kinematics and the stellar populations of the bulge and disc of the spiral galaxy NGC 3521.  ...  The youngest population contributes mostly to the disc component and its contribution increases with radius. We also study the luminosity-weighed properties of the stars in NGC 3521.  ...  KINEMATICS AND SPECTRAL DECOMPOSITION The stellar and ionized-gas kinematics of NGC 3521 were initially measured non parametrically in each spatial bin by fitting the observations with a series of stellar  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/sty705">doi:10.1093/mnras/sty705</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/hgdcj7uib5gidbk4kgta7dr36q">fatcat:hgdcj7uib5gidbk4kgta7dr36q</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20191024101210/https://arxiv.org/pdf/1803.03653v1.pdf" title="fulltext PDF download [not primary version]" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <span style="color: #f43e3e;">&#10033;</span> <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/33/0a/330a38c2a83010f959df2d72db3d6c2e6cf4a4f0.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/sty705"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> oup.com </button> </a>

Properties and formation mechanism of the stellar counter-rotating components in NGC 4191

L. Coccato, M. Fabricius, L. Morelli, E. M. Corsini, A. Pizzella, P. Erwin, E. Dalla Bontà, R. Saglia, R. Bender, M. Williams
<span title="">2015</span> <i title="EDP Sciences"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/hn2qalwlofhybedfhzkh4ogcn4" style="color: black;">Astronomy and Astrophysics</a> </i> &nbsp;
We also performed a photometric decomposition, modelling the galaxy with a S\'ersic bulge and two exponential disks of different scale length, with the aim of associating these structural components with  ...  The two kinematic stellar components counter-rotate with respect to each other.  ...  To obtain a reasonable and stable fit for the special case of NGC 4191, it is necessary to constrain the flux ratio of the two kinematic components by performing an independent photometric decomposition  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/0004-6361/201526560">doi:10.1051/0004-6361/201526560</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/fxy2cwep7nb6xkseigszzy5ysa">fatcat:fxy2cwep7nb6xkseigszzy5ysa</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180726001150/https://www.aanda.org/articles/aa/pdf/2015/09/aa26560-15.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/69/ca/69ca3e4eafff4ff28bef766677c20a702d791949.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/0004-6361/201526560"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Untangling galaxy components: full spectral bulge–disc decomposition

Martha Tabor, Michael Merrifield, Alfonso Aragón-Salamanca, Michele Cappellari, Steven P. Bamford, Evelyn Johnston
<span title="2016-12-09">2016</span> <i title="Oxford University Press (OUP)"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/qjdxzupqgjennounydm4zfdlem" style="color: black;">Monthly notices of the Royal Astronomical Society</a> </i> &nbsp;
These decompositions allow us to study the kinematic and stellar population properties of the individual components and how they vary with position, in order to assess their plausibility as discrete elements  ...  and disk components, subject only to the constraint that they reproduce the conventional photometric decomposition.  ...  NGC 528 In order to determine the kinematics of the bulge and disc implied by the assumed bulge-disc photometric decomposition, we have fitted each Voronoi bin with a kinematic model comprising two components  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stw3183">doi:10.1093/mnras/stw3183</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/lwihopud5baqfapgqxfrug2z2i">fatcat:lwihopud5baqfapgqxfrug2z2i</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180720035829/http://eprints.nottingham.ac.uk/40045/1/stw3183.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/3e/d6/3ed624383956829cdd7f5e4527cd594fdc3d0a6a.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stw3183"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> oup.com </button> </a>

SDSS IV MaNGA: Full spectroscopic bulge-disc decomposition of MaNGA early-type galaxies

Martha Tabor, Michael Merrifield, Alfonso Aragón-Salamanca, Amelia Fraser-McKelvie, Thomas Peterken, Rebecca Smethurst, Niv Drory, Richard R Lane
<span title="2019-02-13">2019</span> <i title="Oxford University Press (OUP)"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/qjdxzupqgjennounydm4zfdlem" style="color: black;">Monthly notices of the Royal Astronomical Society</a> </i> &nbsp;
By applying spectroscopic decomposition methods to a sample of MaNGA early-type galaxies, we separate out spatially and kinematically distinct stellar populations, allowing us to explore the similarities  ...  The resulting components exhibit kinematic parameters consistent with those from the spectroscopic decomposition, and though the dynamical modelling suffers from some degeneracies, the bulges and discs  ...  The kinematic decomposition is then performed by fitting each bin in the galaxy with two model spectra.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stz431">doi:10.1093/mnras/stz431</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/obttjt7psveevnme5fsgln2b4m">fatcat:obttjt7psveevnme5fsgln2b4m</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20200922212428/https://arxiv.org/pdf/1902.03792v1.pdf" title="fulltext PDF download [not primary version]" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <span style="color: #f43e3e;">&#10033;</span> <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/6e/76/6e76ae0e933ef9daed42f04e4650874c492715c4.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stz431"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> oup.com </button> </a>

Black Hole Mass Estimates from Reverberation Mapping and from Spatially Resolved Kinematics

Karl Gebhardt, John Kormendy, Luis C. Ho, Ralf Bender, Gary Bower, Alan Dressler, S. M. Faber, Alexei V. Filippenko, Richard Green, Carl Grillmair, Tod R. Lauer, John Magorrian (+3 others)
<span title="2000-11-01">2000</span> <i title="IOP Publishing"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/otgg2yqymve23nrsflax26msgm" style="color: black;">Astrophysical Journal</a> </i> &nbsp;
Reverberation mapping can now be applied with increased confidence to galaxies whose active nuclei are too bright or whose distances are too large for BH searches based on spatially resolved kinematics  ...  kinematics of nearby normal galaxies.  ...  Nevertheless, even using the best kinematic data, Ho (1999) finds that M ¯values from reverberation mapping are still low by a factor of 5 compared with masses based on spatially resolved kinematics  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1086/318174">doi:10.1086/318174</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/2hf5uzj32zb7pksmcmdklnwq2a">fatcat:2hf5uzj32zb7pksmcmdklnwq2a</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180726174533/http://cds.cern.ch/record/446636/files/0007123.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/06/8f/068fde0d2a594847efa714391cf1f6ec54036ead.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1086/318174"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> iop.org </button> </a>

Hybrid Scheme of Kinematic Analysis and Lagrangian Koopman Operator Analysis for Short-term Precipitation Forecasting [article]

Shitao Zheng, Takashi Miyamoto, Koyuru Iwanami, Shingo Shimizu, Ryohei Kato
<span title="2020-06-03">2020</span> <i > arXiv </i> &nbsp; <span class="release-stage" >pre-print</span>
With the accumulation of meteorological big data, data-driven models for short-term precipitation forecasting have shown increasing promise.  ...  The advection currents are estimated by kinematic analysis, and the changes in physical quantities are estimated by Koopman operator analysis.  ...  These results occurred because the advected precipitation area was expressed with a spatially fixed mode in fugure 5, whereas the results in Figure 6 , where mode decomposition was applied to data whose  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2006.02064v1">arXiv:2006.02064v1</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/gu2a35keq5gknogc3ehssxtyd4">fatcat:gu2a35keq5gknogc3ehssxtyd4</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20200910174949/https://arxiv.org/pdf/2006.02064v1.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/03/ef/03ef539e211567edc3e04b8e8163ba276db141d8.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2006.02064v1" title="arxiv.org access"> <button class="ui compact blue labeled icon button serp-button"> <i class="file alternate outline icon"></i> arxiv.org </button> </a>

Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey – II. Size–luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass

Connor Bottrell, Paul Torrey, Luc Simard, Sara L. Ellison
<span title="2017-02-03">2017</span> <i title="Oxford University Press (OUP)"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/qjdxzupqgjennounydm4zfdlem" style="color: black;">Monthly notices of the Royal Astronomical Society</a> </i> &nbsp;
In this second paper in a series, we employ bulge+disc decompositions of realistic dust-free galaxy images from the Illustris simulation in a consistent comparison with galaxies from the Sloan Digital  ...  We show that photometric bulge fractions are systematically lower than the kinematic fractions at low masses, but with increasingly good agreement as the stellar mass increases.  ...  The uncertainties from the distribution of decomposition results are not consistent with the kinematic estimate.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stx276">doi:10.1093/mnras/stx276</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/ekgyrgqtnfck5iu7tvhfs3evaa">fatcat:ekgyrgqtnfck5iu7tvhfs3evaa</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20191014140115/https://arxiv.org/pdf/1701.08206v1.pdf" title="fulltext PDF download [not primary version]" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <span style="color: #f43e3e;">&#10033;</span> <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/a8/b4/a8b475f3b4813e5842da28141e17838267475001.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stx276"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> oup.com </button> </a>

The dark matter halo shape of edge-on disk galaxies

J. C. O'Brien, K. C. Freeman, P. C. van der Kruit
<span title="">2010</span> <i title="EDP Sciences"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/hn2qalwlofhybedfhzkh4ogcn4" style="color: black;">Astronomy and Astrophysics</a> </i> &nbsp;
To calculate the force fields, we need to analyse the observed XV diagrams to accurately measure all three functions that describe the planar kinematics and distribution of a galaxy: the radial HI surface  ...  We will apply this 'radial decomposition XV modelling method' to our HI observations of 8 HI-rich, late-type, edge-on galaxies in the third paper of this series.  ...  Wark for help and advice with data reduction and analysis. We thank the referee, J.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/0004-6361/200912566">doi:10.1051/0004-6361/200912566</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/dr54z6ipcfct5f53ocwvxbz4my">fatcat:dr54z6ipcfct5f53ocwvxbz4my</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20190429131749/https://www.aanda.org/articles/aa/pdf/2010/07/aa12566-09.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/5d/31/5d31dae681207223e35a00b6b0b0d1a2410b633f.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/0004-6361/200912566"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Mode I Crack Propagation under High Cyclic Loading in 316L Stainless Steel

W. Zhang, S. Pommier, F. Curtit, G. Léopold, S. Courtin
<span title="">2014</span> <i title="Elsevier BV"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/jfkhoe7ilbfrpg7w66gf3ujpnq" style="color: black;">Procedia Materials Science</a> </i> &nbsp;
Each field is approached by the product of a spatial reference field and its intensity factor. This approach allows dealing with the crack growth at large-scale.  ...  Non-linear FE analyses were used to show that such an approximation is reasonably precise.  ...  kinematic behaviour.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1016/j.mspro.2014.06.195">doi:10.1016/j.mspro.2014.06.195</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/iw6gv27wrrawdh6iojycukehyy">fatcat:iw6gv27wrrawdh6iojycukehyy</a> </span>
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The stellar metallicity distribution of disc galaxies and bulges in cosmological simulations

F. Calura, B. K. Gibson, L. Michel-Dansac, G. S. Stinson, M. Cignoni, A. Dotter, K. Pilkington, E. L. House, C. B. Brook, C. G. Few, J. Bailin, H. M. P. Couchman (+1 others)
<span title="2012-11-19">2012</span> <i title="Oxford University Press (OUP)"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/qjdxzupqgjennounydm4zfdlem" style="color: black;">Monthly notices of the Royal Astronomical Society</a> </i> &nbsp;
After undertaking a kinematic decomposition of each simulation into spheroid and disc sub-components, we compare the predicted MDFs to those observed in the solar neighbourhood and the Galactic bulge.  ...  Possible reasons for this apparent discrepancy include the use of low stellar yields and/or centrally-concentrated star formation.  ...  ) after a kinematic decomposition plus a spatial cut as described in Section 2.3.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1111/j.1365-2966.2012.22052.x">doi:10.1111/j.1365-2966.2012.22052.x</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/3rmfxdnb7jco5b3wwflj3miqsa">fatcat:3rmfxdnb7jco5b3wwflj3miqsa</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20170818044946/https://deepblue.lib.umich.edu/bitstream/handle/2027.42/94466/mnr22052.pdf?sequence=1" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/08/e9/08e9c86a5302d111e9884ba4fea42e9cf875f25e.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1111/j.1365-2966.2012.22052.x"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Galaxy Kinematics with SALT [article]

Matthew A. Bershady, Marc A. W. Verheijen , Rob A. Swaters, Kyle B. Westfall (University of Wisconsin)
<span title="2004-03-19">2004</span> <i > arXiv </i> &nbsp; <span class="release-stage" >pre-print</span>
Bi-dimensional kinematic measurements have been the stumbling block.  ...  The light-gathering power of SALT coupled with the high-throughput performance of the Prime Focus Imaging Spectrograph (PFIS) yield a superb facility for measuring velocity-ellipsoids of stars and gas  ...  Galaxy Kinematics with SALT 3 Figure 2 .  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/astro-ph/0403478v1">arXiv:astro-ph/0403478v1</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/wzrxnh547rczzjjn2noo5uj5sy">fatcat:wzrxnh547rczzjjn2noo5uj5sy</a> </span>
<a target="_blank" rel="noopener" href="https://archive.org/download/arxiv-astro-ph0403478/astro-ph0403478.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> File Archive [PDF] </button> </a> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/astro-ph/0403478v1" title="arxiv.org access"> <button class="ui compact blue labeled icon button serp-button"> <i class="file alternate outline icon"></i> arxiv.org </button> </a>

Comparative verification into gait motion of healthy subjects and trans-femoral amputee based on singular value decomposition

Y. Hayashi, N. Tsujiuchi, T. Koizumi, Y. Matsuda
<span title="">2014</span> <i title="IEEE"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/yeqgyhsx6ngq3a5unolasvcire" style="color: black;">5th IEEE RAS/EMBS International Conference on Biomedical Robotics and Biomechatronics</a> </i> &nbsp;
In this paper, joint angles as kinematic parameters applied on the lower limb of healthy subjects and trans-femoral amputee with the prosthetic limb during their gait locomotion are analyzed by singular  ...  value decomposition and mutual comparative verification of them is performed.  ...  in Fig. 14 and Fig. 18 for the same reason.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1109/biorob.2014.6913914">doi:10.1109/biorob.2014.6913914</a> <a target="_blank" rel="external noopener" href="https://dblp.org/rec/conf/biorob/HayashiTKM14.html">dblp:conf/biorob/HayashiTKM14</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/pecgacqanndnfdckk4xn4rkt4u">fatcat:pecgacqanndnfdckk4xn4rkt4u</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20170812011818/http://vigir.missouri.edu/~gdesouza/Research/Conference_CDs/BioRob_2014/media/files/0097.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/99/ee/99eec8f196aeb6a85ff765abe0ec589d6e1522c1.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1109/biorob.2014.6913914"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> ieee.com </button> </a>

Baryonic distributions in galaxy dark matter haloes – I. New observations of neutral and ionized gas kinematics

Emily E. Richards, L. van Zee, K. L. Barnes, S. Staudaher, D. A. Dale, T. T. Braun, D. C. Wavle, J. J. Dalcanton, J. S. Bullock, R. Chandar
<span title="2016-04-29">2016</span> <i title="Oxford University Press (OUP)"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/qjdxzupqgjennounydm4zfdlem" style="color: black;">Monthly notices of the Royal Astronomical Society</a> </i> &nbsp;
The HI rotation curves are supplemented with optical spectroscopic integral field unit (IFU) observations using SparsePak on the WIYN 3.5 m telescope to constrain the central ionized gas kinematics in  ...  Differences in the inferred distribution of mass are illustrated under fixed stellar mass-to-light ratio (M/L) and maximum disc/bulge assumptions in the rotation curve decomposition.  ...  The maximum disc decomposition with M/L = 0.8 provides an equally reasonable fit to the observed rotation curve.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stw1016">doi:10.1093/mnras/stw1016</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/npco7bbwcvc3ncblz5gkxxkj24">fatcat:npco7bbwcvc3ncblz5gkxxkj24</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20191016142145/https://arxiv.org/pdf/1605.01638v1.pdf" title="fulltext PDF download [not primary version]" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <span style="color: #f43e3e;">&#10033;</span> <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/79/fa/79faefb0b8c468aabec7d06dcf5ebfa5fbf03c36.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/stw1016"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> oup.com </button> </a>

Interpreting the kinematics of the extended gas in distant radiogalaxies from 8-10 m telescope spectra

M. Villar-Martín, A. Alonso-Herrero, S. di Serego Alighieri, J. Vernet
<span title="">2000</span> <i title="EDP Sciences"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/dgqnqxsjofgehfjovvnd3odbve" style="color: black;">Astronomy and Astrophysics Supplement Series</a> </i> &nbsp;
We propose to extend the methods applied to low redshift radio galaxies to investigate the nature of the kinematics in distant radio galaxies: by means of the spectral decomposition of the strong optical  ...  If shocks are responsible for the extreme kinematics, we should be able to isolate a kinematic component (the shocked gas) with large FWHM (>900 km/s), low ionization level [OIII]5007/Hb~2-4 and weak HeII4686  ...  We propose that the joint study of the line kinematics (with spectral decomposition of the line profiles) and the line ratios may give the answer.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/aas:2000303">doi:10.1051/aas:2000303</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/quqkai7k7vc35fvuahbj2iqhnq">fatcat:quqkai7k7vc35fvuahbj2iqhnq</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20170808231946/https://aas.aanda.org/articles/aas/pdf/2000/20/ds1884.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] <div class="menu fulltext-thumbnail"> <img src="https://blobs.fatcat.wiki/thumbnail/pdf/6c/f9/6cf90331c30989859c8882545cea201f58cab691.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/aas:2000303"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Modal Decompositions of the Kinematics of Crevalle Jack and the Fluid-Caudal Fin Interaction [article]

Muhammad Saif Ullah Khalid, Junshi Wang, Imran Akhtar, Haibo Dong, Moubin Liu
<span title="2020-05-18">2020</span> <i > arXiv </i> &nbsp; <span class="release-stage" >pre-print</span>
of complex kinematics of a Crevalle Jack (Caranx hippos) fish.  ...  In this paper, we employ advanced modal decomposition techniques; proper orthogonal decomposition and dynamic mode decomposition, to extract energetically strongest spatio-temporal orthonormal components  ...  Using POD technique, we decompose its full-order kinematics into its spatially orthonormal modes.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2005.08589v1">arXiv:2005.08589v1</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/7cww7lymujahfpsve3ugqyzdhm">fatcat:7cww7lymujahfpsve3ugqyzdhm</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20200527071031/https://arxiv.org/ftp/arxiv/papers/2005/2005.08589.pdf" title="fulltext PDF download" data-goatcounter-click="serp-fulltext" data-goatcounter-title="serp-fulltext"> <button class="ui simple right pointing dropdown compact black labeled icon button serp-button"> <i class="icon ia-icon"></i> Web Archive [PDF] </button> </a> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2005.08589v1" title="arxiv.org access"> <button class="ui compact blue labeled icon button serp-button"> <i class="file alternate outline icon"></i> arxiv.org </button> </a>
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