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On the Absorption of X-Rays in the Interstellar Medium
DOI: 10.1086/317016 Bibcode: 2000ApJ...542..914W

McCray, R.; Wilms, J.; Allen, A.

We present an improved model for the absorption of X-rays in the interstellar medium (ISM) intended for use with data from future X-ray missions with larger effective areas and increased energy resolution such as Chandra and the X-Ray Multiple Mirror mission, in the energy range >~100 eV. Compared with previous work, our formalism includes rece…

2000 The Astrophysical Journal
XMM-Newton 3343
Thomson Thick X-Ray Absorption in a Broad Absorption Line Quasar, PG 0946+301
DOI: 10.1086/312617 Bibcode: 2000ApJ...533L..79M

Arav, N.; Elvis, M.; Peterson, B. M. +14 more

We present a deep ASCA observation of a broad absorption line quasar (BALQSO) PG 0946+301. The source was clearly detected in one of the gas imaging spectrometers, but not in any other detector. If BALQSOs have intrinsic X-ray spectra similar to normal radio-quiet quasars, our observations imply that there is Thomson thick X-ray absorption (N

2000 The Astrophysical Journal
XMM-Newton 45
Detection of the Entropy of the Intergalactic Medium: Accretion Shocks in Clusters, Adiabatic Cores in Groups
DOI: 10.1086/309500 Bibcode: 2000ApJ...542..106T

Tozzi, Paolo; Norman, Colin; Scharf, Caleb

The thermodynamics of the diffuse, X-ray-emitting gas in clusters of galaxies is linked to the entropy level of the intracluster medium. In particular, models that successfully reproduce the properties of local X-ray clusters and groups require the presence of a minimum value for the entropy in the center of X-ray halos. Such a minimum entropy is …

2000 The Astrophysical Journal
XMM-Newton 43
Probing Cosmology with the X-Ray Forest
DOI: 10.1086/309270 Bibcode: 2000ApJ...539..532F

Canizares, Claude R.; Fang, Taotao

There is a growing consensus that in the present universe most baryons reside in galaxy clusters and groups in the form of highly ionized gas at temperatures of 106-108 K. The H-like and He-like ions of the heavy elements can produce absorption features-the so-called ``X-ray forest''-in the X-ray spectrum of a background quas…

2000 The Astrophysical Journal
XMM-Newton 34