Modeling the redshift evolution of the normal galaxy x-ray luminosity function

Astrophysical Journal

Volumn 766, Issue 1, 2013, Pages

  Tremmel, M ^a   Fragos, T ^b   Lehmer, B D ^c,d   Tzanavaris, P ^c,d   Belczynski, K ^e,f   Kalogera, V ^g   Basu Zych, A R ^d   Farr, W M ^g   Hornschemeier, A ^d   Jenkins, L ^d   Ptak, A ^d   Zezas, A ^b,h,i  

^a UNIVERSITY OF WASHINGTON   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e UNIVERSITY OF WARSAW   (Poland)

^f UNIVERSITY OF TEXAS AT BROWNSVILLE   (United States)

^g NORTHWESTERN UNIVERSITY   (United States)

^h UNIVERSITY OF CRETE   (Greece)

ⁱ INSTITUTE OF ELECTRONIC STRUCTURE AND LASER   (Greece)

Author keywords

binaries: close; galaxies: stellar content; stars: evolution; X rays: binaries; X rays: diffuse background; X rays: galaxies

Indexed keywords

EID: 84875026460     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/766/1/19     Document Type: Article

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