Expectations for X-Ray-Cluster Observations by the Rosat Satellite
dc.contributor.author | Evrard, August E. | en_US |
dc.contributor.author | Henry, J. P. | en_US |
dc.date.accessioned | 2008-08-14T19:12:50Z | |
dc.date.available | 2008-08-14T19:12:50Z | |
dc.date.issued | 1991-12-10 | en_US |
dc.identifier.citation | Evrard, AE; Henry, JP. (1991). Astrophysical Journal, 383:(1, Part1) 95-103. <http://hdl.handle.net/2027.42/60621> | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/60621 | |
dc.description.abstract | We present predictions for characteristics of the X-ray cluster population expected to be observed by the ROSAT satellite. The theoretical modeling requires an assumed fluctuation spectrum and relations describing the behavior of cluster X-ray luminosity and core radius with cluster binding mass and redshift. The most natural model, which assumes self-similar scaling L(x) is-proportional-to M4/3 in a cold dark matter (CDM) universe, fails to reproduce the shape of the local X-ray cluster luminosity function. For CDM to be successful, the bolometric X-ray luminosity L(x) must scale with binding mass M as L(x) is-proportional-to M3, perhaps indicative of a strong dependence of intracluster gas fraction with mass. An alternative model motivated by recent evidence for more large-scale power, uses an n = -2 initial fluctuation spectrum and fits local cluster abundances with an intermediate scaling L(x) is-proportional-to M11/6. This scaling law may imply a fixed minimum entropy for the gas in the cores of rich clusters, perhaps a signature of activity from an earlier galaxy formation era. For the north ecliptic pole region of the ROSAT all-sky survey, which will cover a 10-degrees radius field to a limiting flux of roughly 9 x 10(-14) ergs s-1 cm-2, the successful models predict approximately 330 cluster X-ray sources visible above the flux limit if a square detect cell of side 4'8 is employed. The clusters would have a median redshift of 0.2, and 10% of them should have z > 0.4 but essentially none should be seen at z > 1. Roughly 2500 clusters are expected with this detect geometry in the all-sky survey above the limiting flux of 7 x 10(-13) ergs s-1 cm-2. Cluster sources would be expected to contribute approximately 10% of the observed soft X-ray background. The sensitivity of cluster detectability to treatment of the core emission and detect cell geometry is the principal source of uncertainty in these predictions. | en_US |
dc.format.extent | 1527299 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 | Dark Matter | en_US |
dc.subject | Galaxies : Clustering | en_US |
dc.subject | Galaxies : X-rays | en_US |
dc.title | Expectations for X-Ray-Cluster Observations by the Rosat Satellite | 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.affiliationother | MAX PLANCK INST EXTRATERRESTR PHYS,W-8046 GARCHING,GERMANY | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/60621/1/1991ApJ___383___95E.pdf | |
dc.identifier.doi | http://dx.doi.org/10.1086/170767 | en_US |
dc.owningcollname | Astrophysics (Physics, Department of) |
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