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It illustrates the process by obtaining remnants from: Google Docs accessed by Internet Explorer, Dropbox, and Windows Live Mesh. Identifying Remnants of Evidence in the Cloud 43 the world. ... With the advent of cloud computing, law enforcement investigators are facing the challenge that instead of the evidence being on a device that they can seize, the evidence is likely located in remote data ... Identifying Cloud Signature Remnants To identify cloud application remnant data sets we first identify which files the cloud applications typically install and/or access, then we use software to parse ...doi:10.1007/978-3-642-39891-9_3 fatcat:w3tevyqhcfcbxhrarejflhxpuu
Using pCloud as a case study, this research collected the data remnants available on end-user device storage following the storing, uploading, and accessing of data in the cloud storage. ... Results demonstrate that the collected remnants data is beneficial in determining a sufficient number of artifacts about the investigated cyber crime. ... An evidence locating process identified the location of each file change. This process served as a guideline in locating potential data remnants being stored. ...doi:10.1111/1556-4029.13506 pmid:28397244 fatcat:bnyciwd6wzh3rpfdvyfxu462ki
Imaging and spectral observations in the X-ray band can be used to identify properties of the remnants that lead to gamma-ray emission, including the presence of pulsar-driven nebulae, nonthermal X-ray ... The mechanisms by which such gamma-rays can arise may include emission from a pulsar associated with a remnant, or a variety of processes associated with energetic particles accelerated by the SNR shock ... This work was supported in part by NASA through contract NAS8-39073 and grants NAG5-9106 and NAG5-9281. ...arXiv:astro-ph/0104348v1 fatcat:jygu43pgzzde5eif6nlndg3kua
Astrophysics and Space Science Library
Imaging and spectral observations in the X-ray band can be used to identify properties of the remnants that lead to γ-ray emission, including the presence of pulsar-driven nebulae, nonthermal X-ray emission ... The mechanisms by which such γ-rays can arise may include emission from a pulsar associated with a remnant, or a variety of processes associated with energetic particles accelerated by the SNR shock. ... This work was supported in part by NASA through contract NAS8-39073 and grants NAG5-9106 and NAG5-9281. ...doi:10.1007/978-94-010-1007-8_16 fatcat:rpuxyi52ljggfklmc5tbg6zz4i
Astronomy and Astrophysics
The observations can give direct evidence, through the morphology, the shape, of the remnants (see Sect. 2.1). ... Astrophys. 174, 5-12 (1987) ASTRONOMY AND ASTROPHYSICS Model calculations for supernova remnants in the Large Magellanic Cloud M. ...
When misused as a tool of crimes, investigators can expect to find evidence and traces of criminal activity in both local system and cloud providers. ... This increased adoption of cloud storage had amplified the demand for cloud forensics, the cross-discipline between cloud computing and digital forensics. ... Since cloud is where the evidence resides, cloud is now the digital evidence which need to be preserved and acquired. ...doi:10.14445/22315381/cati3p207 fatcat:7ab23gwa2jagnjs653fglewmky
The flux of photons with energies above 1 TeV from the direction of the centre and a cloud in the western part of the nearby southern supernova remnant (SNR) RX J1713.7-3946 is calculated in the "hadronic ... While the size of this discrepancy might still seem acceptable in the face of various theoretical uncertainties, the result strongly suggests a strict spatial correlation of the cloud with an excess of ... Acknowledgements I thank Werner Hofmann, Alvaro de Rujula and an anonymous referee for critical remarks on a previous version of this paper, that helped to improve it significantly. ...doi:10.1016/j.newast.2007.06.005 fatcat:c65bnzfefzaulfkwexf4kp5rre
There are a half-dozen or so young supernova remnants in the Magellanic Clouds that display one or more of the following characteristics: high velocity (>1000 km/s) emission, enhanced metallicity, or a ... I summarize the current state of knowledge of these remnants and present some recent results mostly from the new X-ray astronomy satellites. ... Acknowledgments I gratefully acknowledge Dave Burrows, Anne Decourchelle, Gordon Garmire, Parviz Ghavamian, Karen Lewis, John Nousek, Cara Rakowski, and Pat Slane for their collaborations on various studies of ...doi:10.1063/1.1377130 fatcat:2islrozba5cmjopoply5ysyhuq
Astronomy and Astrophysics
The remnant of the SN is still embedded in the cloud, and cannot be observed due to extinction. ... We assume that the SN exploded in the molecular cloud p Oph in the 14th century B.C.; the cosmic rays were generated during the initial stage of the evolution of the remnant. ...
We present the results of GBT observations of all four ground-state hydroxyl (OH) transitions toward 15 supernova remnants (SNRs) which show OH(1720 MHz) maser emission. ... We infer that spatially extended, low level maser emission is a common phenomenon that traces the large-scale interaction in maser-emitting SNRs. ... A comparison with VLA detections in the literature allows us to identify which remnants show evidence for maser emission being resolved out by the interferometer. ...doi:10.1086/588652 fatcat:v3xq7byzs5hcvicxhefzxvkaiq
A considerable fraction of them may most probably be formed by an interaction between supernova remnants (SNRs) and molecular clouds. ... Studies of such cases in less confused areas are needed to clarify this picture. The SNR W44 is a good place for examining the SNR induced shell formation scenario. ... We established W44 as first unambiguously identified example interaction between the SNR and Giant molecular cloud based on following evidences of interaction: MASUMICHI SETA ET AL. 1) coincidence in position ...doi:10.1017/s0074180900084606 fatcat:c44aztlf6zgd5hual7sjm7v32y
In today society where we live in a world of constant connectivity, many people are now looking to cloud services in order to store their files so they can have access to them wherever they are. ... From a forensics perspective, the increasing popularity of cloud storage platforms, makes investigation into such exploits much more difficult, especially since many platforms such as mobile devices as ... Additionally, a remnant of the page title was found in memory ( Figure 5 ). C. ...doi:10.1109/cloudcom.2015.24 dblp:conf/cloudcom/BlakeleyCDA15 fatcat:onkdevjzc5girlijtlogpffeti
Supernova remnants interacting with molecular clouds are potentially exciting systems in which to detect evidence of cosmic ray acceleration. ... In many of the supernova remnants coincident with gamma-ray sources, the presence of OH(1720 MHz) masers is used to identify interaction with dense gas and to provide a kinematic distance to the system ... Of the 26 remnants for which an association with the coincident γ -ray source has not been ruled out, 7 are young remnants ( 1 kyr), 12 are SNRs with evidence of interaction with dense clouds, and 7 are ...doi:10.1088/0004-637x/706/2/l270 fatcat:gextsgwtmrdndjfysp3ldtxo34
Astronomy and Astrophysics
Combining near infrared, IRAS and millimetric molecular line data we have identified the brightest members of the Class I population in the Vela molecular clouds. 2. ... Given the available observational evidence we exclude the possibility that star formation in the VMR has been induced by the recent detonation of a supernova. 7. ...
A list is presented of about 80 objects of these remnant clouds in the Ori OB 1 association. ... We suspect that retarded star formation in remnant clouds can explain the presence of so-called dispersed T Tau stars in the peripheries of OB associations. ... Table 1 summarises the results. The first column gives the object number identified in Figure 1 . The second and third columns contain the 1950 coordinates of the cloud centre. ...doi:10.1071/as98091 fatcat:nwq3mpxez5gedkh66ks3je4oti
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