The faint X-ray source population near 3C 295

Astronomy and Astrophysics

Volumn 422, Issue 1, 2004, Pages 11-21

  D'Elia, V ^a   Fiore, F ^a   Elvis, M ^b   Cappi, M ^c   Mathur, S ^d   Mazzotta, P ^e   Falco, E ^f   Cocchia, F ^a  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c CNR   (Italy)

^d OHIO STATE UNIVERSITY   (United States)

^e DURHAM UNIVERSITY   (United Kingdom)

^f SMITHSONIAN INSTITUTION   (United States)

Author keywords

Cosmology: large scale structure of universe; Galaxies: clusters: individual: 3C 295; X rays: Diffuse background; X rays: galaxies

Indexed keywords

CORRELATION METHODS; EXTRATERRESTRIAL ATMOSPHERES; GALAXIES; GASES; LIGHT EMISSION; X RAY ANALYSIS;

ANGULAR CORRELATION FUNCTION (ACF); COSMOLOGY; SPATIAL CORRELATION;

ASTROPHYSICS;

EID: 3142674206     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040149     Document Type: Article

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