Detecting intracluster gas motion in galaxy clusters: Mock Astro-E2 observations
dc.contributor.author | Pawl, Andrew | en_US |
dc.contributor.author | Evrard, August E. | en_US |
dc.contributor.author | Dupke, Renato A. | en_US |
dc.date.accessioned | 2008-08-14T19:10:18Z | |
dc.date.available | 2008-08-14T19:10:18Z | |
dc.date.issued | 2005-10-01 | en_US |
dc.identifier.citation | Pawl, A; Evrard, AE; Dupke, RA. (2005). Astrophysical Journal, 631:(2, Part1) 773-784. <http://hdl.handle.net/2027.42/60578> | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://arxiv.org/abs/astro-ph/0503281 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/60578 | |
dc.description.abstract | We explore the detectability of bulk motions in the X-ray-emitting intracluster medium using a catalog of 1836 mock Astro-E2 observations of simulated clusters of galaxies. We generate high-resolution mock spectra for two observing strategies: a four-pointing mosaic and a single central pointing. Normalizing to 200 ( 400) photons in the iron K alpha region for the mosaic ( central) study, we fit Poisson realizations of each simulated spectrum to a velocity-broadened isothermal plasma emission model. We confirm that the velocity characteristics ( mean and dispersion) returned by the spectral fittings are unbiased measures of the emission-weighted values within the observed region, with scatter +/- 55 km s(-1). The maximum velocity difference between mosaic element pairs Delta nu(max) has similar to 6% likelihood of being transonic (Delta nu(max) >= 0.5c(s)), and the likelihood falls steeply, p proportional to (Delta nu(max)/c(s))(-4), at high Mach number. The velocity-broadening parameter sigma(nu) from the central pointing fit exceeds the thermal value in 49% of the cases, with again a sigma(nu)(-4) tail at large dispersion. We present as case studies the clusters that yield the strongest signal for each observing strategy. | en_US |
dc.format.extent | 297050 bytes | |
dc.format.extent | 18 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.publisher | Univ Chicago Press | en_US |
dc.subject | Cosmology : Observations | en_US |
dc.subject | Galaxies : Clusters : General | en_US |
dc.subject | Intergalactic Medium | en_US |
dc.subject | X-rays : Galaxies : Clusters | en_US |
dc.title | Detecting intracluster gas motion in galaxy clusters: Mock Astro-E2 observations | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Univ Michigan, Michigan Ctr Theoret Phys, Ann Arbor, MI 48109 USA | en_US |
dc.contributor.affiliationum | Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA | en_US |
dc.contributor.affiliationum | Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/60578/1/Pawl2005Detecting.pdf | |
dc.identifier.doi | http://dx.doi.org/10.1086/432608 | en_US |
dc.owningcollname | Astrophysics (Physics, Department of) |
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