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Multiwavelength Observations of Relativistic Jets from General Relativistic Magnetohydrodynamic Simulations

Richard Anantua, Roger Blandford, Alexander Tchekhovskoy
<span title="2018-03-03">2018</span> <i title="MDPI AG"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/t4jq7k6xuraorp476xxuark3wi" style="color: black;">Galaxies</a> </i> &nbsp;
Synthetic observations can be directly compared with real observations for observational signatures such as jet instabilities, collimation, relativistic beaming, and polarization.  ...  This work summarizes a program intended to unify three burgeoning branches of the high-energy astrophysics of relativistic jets: general relativistic magnetohydrodynamic (GRMHD) simulations of ever-increasing  ...  In the observation in Figure 1 , M87 has a distinctive swirling pattern, possibly indicative of magnetic Kelvin-Helmholtz or kink instability.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.3390/galaxies6010031">doi:10.3390/galaxies6010031</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/wh2dgydl3zdzxeuev46at55l54">fatcat:wh2dgydl3zdzxeuev46at55l54</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180724140152/https://res.mdpi.com/def50200bbeead5bf552964f50c4e9172aae2ba3f7aa361177a455cc0731b769a113aee95ad4383e6ead9d830034be43232d757c4c27c276e71ab0f5cf054523e5fce5d9de4a3e872199d2c3da50a5288ce9414c46f2afdcca35dd83fc47ee9c1a69bbab65e36dfebd83c219c4383f1c3e3e100240f90d6bea1a32e2051ce96ead705142ebe47c3112fb37e6f150bfde85b4790eb4d2?filename=&amp;attachment=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/6b/99/6b992f70c87fa037e39cc432064cb53c58f010f4.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.3390/galaxies6010031"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="unlock alternate icon" style="background-color: #fb971f;"></i> mdpi.com </button> </a>

Numerical study of Kelvin-Helmholtz instability and its impact on synthetic emission from magnetized jets [article]

Nikhil Borse, Sriyasriti Acharya, Bhargav Vaidya, Dipanjan Mukherjee, Gianluigi Bodo, Paola Rossi, Andrea Mignone
<span title="2021-03-11">2021</span> <i > arXiv </i> &nbsp; <span class="release-stage" >pre-print</span>
We find that the shocks due to Kelvin-Helmholtz (KH) instability in the axial magnetic field configurations can strongly affect the jet dynamics.  ...  macro-particles incorporating the effects of shock acceleration and radiative losses.  ...  Acknowledgements The authors would like to thank the referee for providing valuable comments and helping to improve the manuscript significantly.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2009.13540v2">arXiv:2009.13540v2</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/dtdgif4htzb2vjfvnfkwya5f2u">fatcat:dtdgif4htzb2vjfvnfkwya5f2u</a> </span>
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Thermal material in jets [article]

A. Celotti, M. J. Rees
<span title="1997-07-11">1997</span> <i > arXiv </i> &nbsp; <span class="release-stage" >pre-print</span>
budget, since the thermal reprocessing signatures that should appear in the spectra have not, as yet, been detected.  ...  While the presence of a thermal component occupying a fraction ~1.E-8 of the jet volume is possible, it seems unlikely that such a component is capable of contributing significantly to the total jet energy  ...  ACKNOWLEDGMENTS We acknowledge Gary Ferland for the use of his code CLOUDY. For financial support, thanks are due to the Italian MURST (AC), the Australian DIST (ZK), the Royal Society (MJR).  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/astro-ph/9707132v1">arXiv:astro-ph/9707132v1</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/qbsvnnnzj5gybpdcizywmsn7kq">fatcat:qbsvnnnzj5gybpdcizywmsn7kq</a> </span>
<a target="_blank" rel="noopener" href="https://archive.org/download/arxiv-astro-ph9707132/astro-ph9707132.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/9707132v1" 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>

Thermal material in relativistic jets

A. Celotti, Z. Kuncic, M. J. Rees, J. F. C. Wardle
<span title="1998-01-21">1998</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;
can stabilize relativistic plasma against thermal instability triggered by the presence of localized regions of cool gas.  ...  budget, since the thermal reprocessing signatures that should appear in the spectra have not, as yet, been detected. ᭧ 1998 RAS, MNRAS 293, 288-298 1 Recent observations with the SAX satellite also show  ...  AC K N OW L E D G M E N T S We acknowledge Gary Ferland for the use of his code cloudy.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1046/j.1365-8711.1998.01124.x">doi:10.1046/j.1365-8711.1998.01124.x</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/s2axwv4h2fawhldoagkfabdft4">fatcat:s2axwv4h2fawhldoagkfabdft4</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180729141449/https://watermark.silverchair.com/293-3-288.pdf?token=AQECAHi208BE49Ooan9kkhW_Ercy7Dm3ZL_9Cf3qfKAc485ysgAAAbMwggGvBgkqhkiG9w0BBwagggGgMIIBnAIBADCCAZUGCSqGSIb3DQEHATAeBglghkgBZQMEAS4wEQQMcxPNGQBsEgJcuP98AgEQgIIBZhqz-lqeF8xofM9FUq74O3DAQkMllSPBCelFoZmQfim1l_bKFAXuZ3Y2usuyNs8CvSetvcvX1UKmn6_nS1yQVjt-2gCBmeYChsG8MGoa04kqsCiC9kRbl2SZHBuW8Eau89bgRHGpjBRKkq6ZffPR7sUB7Vs419lJqCgUjY3NTVuFoGjwk9zLCzRbT_1rAXbXrX9c2LDa8elywg9-nKdHxZzVDYODiJRJGjHvwRIh5zMMshnEmXlPCF5ucWNpj0OQ5ATvQM5Pt4Kx-LpzEvkPd2p3ZCfd5VgT0mCFDNKAIC2h7gB-wKmjtUQkGqbeOt4uL0YAvwBckXlV90JeF8gazSVJD_Hi2hqzz7uTIFZNclAodSACCLrGgfLeVXk034lS5RLiA4Ua-aPd2v4NqUg8lniFk5Jb85f49rQ05hsOhQvn89CsmL0fLeXl3pNfgqXR4Pg7EkypxBnISaTwZf1_y2BXaAYrDEc" 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/af/d4/afd45b7a9d60e1c0adb669c719f5b5a69815db94.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1046/j.1365-8711.1998.01124.x"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Jet dynamics and stability

M. Perucho, José L. Gómez
<span title="">2013</span> <i title="EDP Sciences"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/oduy4e4fvfhovftixyndrlkomi" style="color: black;">EPJ Web of Conferences</a> </i> &nbsp;
Pressure asymmetries within the jet may trigger the development of helical patterns via coupling to kink current-driven instability, or to helical Kelvin-Helmholtz instability, depending on the physical  ...  The ridge-line of emission of the jet of S5~0836+710 has been identified as a physical structure corresponding to a wave developing in the jet flow.  ...  Agudo for their work within the projects summarized in these proceedings. This research has made use of data from the MOJAVE database that is maintained by the MOJAVE team [38] .  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/epjconf/20136102002">doi:10.1051/epjconf/20136102002</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/mfygdi6bz5at3hmch63fmjtxpu">fatcat:mfygdi6bz5at3hmch63fmjtxpu</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180722193953/https://www.epj-conferences.org/articles/epjconf/pdf/2013/22/epjconf_rj2013_02002.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/a1/87/a187d5b304a3afe58fc9bbdaf3c8d5a4905e977c.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/epjconf/20136102002"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="unlock alternate icon" style="background-color: #fb971f;"></i> Publisher / doi.org </button> </a>

TOWARD A COMPREHENSIVE MODEL FOR FEEDBACK BY ACTIVE GALACTIC NUCLEI: NEW INSIGHTS FROM M87 OBSERVATIONS BY LOFAR,FERMI, AND H.E.S.S

Christoph Pfrommer
<span title="2013-11-18">2013</span> <i title="IOP Publishing"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/otgg2yqymve23nrsflax26msgm" style="color: black;">Astrophysical Journal</a> </i> &nbsp;
Feedback by active galactic nuclei (AGNs) appears to be critical in balancing radiative cooling of the low-entropy gas at the centers of galaxy clusters and in mitigating the star formation of elliptical  ...  However, the resulting global thermal equilibrium is locally unstable and allows for the formation of the observed cooling multi-phase medium through thermal instability.  ...  through the action of Kelvin-Helmholtz and Rayleigh-Taylor instabilities.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1088/0004-637x/779/1/10">doi:10.1088/0004-637x/779/1/10</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/k4op6dnntzd2vlwgc57ykp42mu">fatcat:k4op6dnntzd2vlwgc57ykp42mu</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180725180153/http://iopscience.iop.org/article/10.1088/0004-637X/779/1/10/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/48/a9/48a9e9a2424c92661dd39de17491eeec1e96cbd7.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1088/0004-637x/779/1/10"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> iop.org </button> </a>

Buoyant radio plasma in clusters of galaxies

M. Bruggen, C. R. Kaiser
<span title="2001-08-01">2001</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 investigate the evolution of the plasma bubbles as they become subject to Rayleigh-Taylor instabilities.  ...  Radio galaxies are known to inflate lobes of hot relativistic plasmas into the intergalactic medium.  ...  The magnetic field is still aligned with the surface of the torus (see Fig. 6 ) and stabilises it against Rayleigh-Taylor and Kelvin-Helmholtz instabilities.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1046/j.1365-8711.2001.04494.x">doi:10.1046/j.1365-8711.2001.04494.x</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/smempefyynbhrebnqxj2v2vwne">fatcat:smempefyynbhrebnqxj2v2vwne</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180725233619/http://cds.cern.ch/record/466944/files/0010023.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/9e/03/9e03cbbc956213c821d538310c7314a898cf7a38.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1046/j.1365-8711.2001.04494.x"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Diagnosing particle acceleration in relativistic jets

Markus Böttcher, Matthew G. Baring, Edison P. Liang, Errol J. Summerlin, Wen Fu, Ian A. Smith, Parisa Roustazadeh
<span title="">2014</span> <i title="Cambridge University Press (CUP)"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/djnl2eulfjdwxplyqzspykhc2m" style="color: black;">Proceedings of the International Astronomical Union</a> </i> &nbsp;
The resulting magnetic-field configurations and thermal + non-thermal particle distributions are then used to predict multi-wavelength radiative (synchrotron + Compton) signatures of both acceleration  ...  populations in diffusive shock acceleration simulations provides tests of the bulk Comptonization model for the Big Blue Bump observed in the SEDs of several blazars.  ...  & Duffy (2006) ) as such shears are likely to be dissipative due to the Kelvin-Helmholtz instability (Chandrasekhar (1981) ).  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1017/s1743921315002100">doi:10.1017/s1743921315002100</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/vlawr26ojfdrhktt66ruyiad4i">fatcat:vlawr26ojfdrhktt66ruyiad4i</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20200505170759/https://www.cambridge.org/core/services/aop-cambridge-core/content/view/C2B1C113B5B783A0933BA865D685ABCB/S1743921315002100a.pdf/div-class-title-diagnosing-particle-acceleration-in-relativistic-jets-div.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/26/52/2652fed3ea1e4b9f7d79ce22dbc756b17e63c3ef.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1017/s1743921315002100"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> cambridge.org </button> </a>

Simulating the dynamics and non-thermal emission of relativistic magnetised jets I. Dynamics [article]

Dipanjan Mukherjee, Gianluigi Bodo, Andrea Mignone, Paola Rossi, Bhargav Vaidya
<span title="2020-09-22">2020</span> <i > arXiv </i> &nbsp; <span class="release-stage" >pre-print</span>
We find that two dominant MHD instabilities affect the dynamics of the jet, small scale Kelvin- Helmholtz (KH) modes and large scale kink modes, whose evolution depend on internal jet parameters like the  ...  We have performed magneto-hydrodynamic simulations of relativistic jets from supermassive blackholes over a few tens of kpc for a range of jet parameters.  ...  and Kelvin-Helmholtz modes.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2009.10475v1">arXiv:2009.10475v1</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/zcbwvihms5f4bifyhc4edvh6di">fatcat:zcbwvihms5f4bifyhc4edvh6di</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20200928144253/https://arxiv.org/pdf/2009.10475v1.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/2009.10475v1" 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>

Simulating the dynamics and synchrotron emission from relativistic jets II. Evolution of non-thermal electrons [article]

Dipanjan Mukherjee, Gianluigi Bodo, Paola Rossi, Andrea Mignone, Bhargav Vaidya
<span title="2021-05-06">2021</span> <i > arXiv </i> &nbsp; <span class="release-stage" >pre-print</span>
However, unstable jets create complex shock structures at the jet-head (kink instability), the jet spine-cocoon interface and the cocoon itself (Kelvin-Helmholtz modes).  ...  The CREs have been evolved in space and in energy concurrently with the relativistic jet fluid, duly accounting for radiative losses and acceleration at shocks.  ...  These vortical motions of the CREs result from the onset of Kelvin-Helmholtz instabilities at the jet-cocoon interface.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2105.02836v1">arXiv:2105.02836v1</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/vf2hnol66bhqhdado67ozrabxm">fatcat:vf2hnol66bhqhdado67ozrabxm</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20211102150051/https://arxiv.org/pdf/2105.02836v2.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/3c/ec/3cec654f4ad6bf2eeef5004f98ae39d052427777.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener" href="https://arxiv.org/abs/2105.02836v1" 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>

STELLAR TIDAL DISRUPTION EVENTS BY DIRECT-COLLAPSE BLACK HOLES

Kazumi Kashiyama, Kohei Inayoshi
<span title="2016-07-25">2016</span> <i title="American Astronomical Society"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/otgg2yqymve23nrsflax26msgm" style="color: black;">Astrophysical Journal</a> </i> &nbsp;
Radiative and mechanical feedback from an inner slim disk and the star cluster will significantly reduce the gas accretion rate onto the DCBH within ∼ 10^6 yr.  ...  Some of the nuclear stars can be scattered onto the loss cone orbits also within ≲ 10^6 yr and tidally disrupted by the central DCBH.  ...  KI is supported by the Simons Foundation through the Simons Society of Fellows.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.3847/0004-637x/826/1/80">doi:10.3847/0004-637x/826/1/80</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/4txttahl75emlbmogxshnmauc4">fatcat:4txttahl75emlbmogxshnmauc4</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20200825162605/https://arxiv.org/pdf/1602.04293v1.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/af/56/af566b01f0fd79879db9659e280c4bf76bead4db.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.3847/0004-637x/826/1/80"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Hydrodynamic Interactions of Relativistic Extragalactic Jets with Dense Clouds

Eunwoo Choi, Paul J. Wiita, Dongsu Ryu
<span title="">2007</span> <i title="IOP Publishing"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/otgg2yqymve23nrsflax26msgm" style="color: black;">Astrophysical Journal</a> </i> &nbsp;
This enhancement of cloud durability is partly due to the geometric influence of the off-axis collisions we consider and also arises from the lower rate of cloud fragmentation through the Kelvin-Helmholtz  ...  instability for relativistic jets.  ...  The simulations were performed on the Linux Biocluster at Georgia State University, and we are grateful for the allocation of substantial time on this cluster.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1086/510120">doi:10.1086/510120</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/6dubyzrkjnaufbaq6uyci2bdya">fatcat:6dubyzrkjnaufbaq6uyci2bdya</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180726223019/http://cds.cern.ch/record/989863/files/0610474.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/74/2a/742ad7a3424361705019cc4478ca649010daf2fc.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1086/510120"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> iop.org </button> </a>

Impact of orbital motion on the structure and stability of adiabatic shocks in colliding wind binaries

A. Lamberts, G. Dubus, G. Lesur, S. Fromang
<span title="">2012</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 focus on adiabatic winds, where mixing between the two winds is expected to be restricted to the Kelvin-Helmholtz instability (KHI).  ...  The collision of winds from massive stars in binaries results in the formation of a double-shock structure with observed signatures from radio to X-rays.  ...  The authors thank the anonymous referee for pointing out the importance of inverse Compton cooling. A.L. and G.D. are supported by the European Community via contract ERC-StG-200911.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/0004-6361/201219006">doi:10.1051/0004-6361/201219006</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/uec3aalyyfay3mwdkw6zpczlx4">fatcat:uec3aalyyfay3mwdkw6zpczlx4</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20180724165232/https://www.aanda.org/articles/aa/pdf/2012/10/aa19006-12.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/0d/c7/0dc7d1b50824fd5115be252f3ce3db23983a9266.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1051/0004-6361/201219006"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> Publisher / doi.org </button> </a>

Numerical Simulations of Jets from Active Galactic Nuclei

José-María Martí
<span title="2019-01-22">2019</span> <i title="MDPI AG"> <a target="_blank" rel="noopener" href="https://fatcat.wiki/container/t4jq7k6xuraorp476xxuark3wi" style="color: black;">Galaxies</a> </i> &nbsp;
The present review summarizes the status of the numerical simulations of jets from AGNs, from the formation region in the neighborhood of the supermassive central black hole up to the impact point well  ...  Numerical simulations have been playing a crucial role in the understanding of jets from active galactic nuclei (AGN) since the advent of the first theoretical models for the inflation of giant double  ...  Conflicts of Interest: The author declares no conflict of interest.  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.3390/galaxies7010024">doi:10.3390/galaxies7010024</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/paqsi46hxfhhre4ptwdvdknw5i">fatcat:paqsi46hxfhhre4ptwdvdknw5i</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20190506022839/https://res.mdpi.com/galaxies/galaxies-07-00024/article_deploy/galaxies-07-00024-v2.pdf?filename=&amp;attachment=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/87/15/8715bdb69baa7dc75e60cb110bc943f946f0dfc6.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.3390/galaxies7010024"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="unlock alternate icon" style="background-color: #fb971f;"></i> mdpi.com </button> </a>

Physical constraints on the sizes of dense clouds in the central magnetospheres of active galactic nuclei

Z. Kuncic, E. G. Blackman, M. J. Rees
<span title="1996-12-11">1996</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;
observable thermal reprocessing signatures.  ...  The range of microphysical and global dynamical timescales in the central regions of Active Galactic Nuclei (AGN) is sufficiently wide to permit the existence of multiphase structure.  ...  ACKNOWLEDGMENTS We thank the referee T. Hartquist for helpful comments. For financial support, thanks are due to the Cambridge Commonwealth Trust (ZK), PPARC (EB) and the Royal Society (MR).  ... 
<span class="external-identifiers"> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/283.4.1322">doi:10.1093/mnras/283.4.1322</a> <a target="_blank" rel="external noopener" href="https://fatcat.wiki/release/6mjglriolvfdbcb5rdjwvi42bu">fatcat:6mjglriolvfdbcb5rdjwvi42bu</a> </span>
<a target="_blank" rel="noopener" href="https://web.archive.org/web/20181030053644/http://cds.cern.ch/record/308976/files/9608104.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/35/ed/35ed66c2921652b341b349aad8a87201eb22d51a.180px.jpg" alt="fulltext thumbnail" loading="lazy"> </div> </button> </a> <a target="_blank" rel="external noopener noreferrer" href="https://doi.org/10.1093/mnras/283.4.1322"> <button class="ui left aligned compact blue labeled icon button serp-button"> <i class="external alternate icon"></i> oup.com </button> </a>
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