Luminosity functions of LMXBs in different stellar environments

Astronomy and Astrophysics

Volumn 533, Issue , 2011, Pages

  Zhang, Z ^a   Gilfanov, M ^a,b   Voss, R ^c   Sivakoff, G R ^d   Kraft, R P ^e   Brassington, N J ^e,f   Kundu, A ^g   Jordan A ^e,h   Sarazin, C ^d  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b Department of Satellite Monitoring Technologies   (Russian Federation)

^c RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^d UNIVERSITY OF VIRGINIA   (United States)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^g EUREKA SCIENTIFIC   (United States)

^h PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

Author keywords

Globular clusters: general; X rays: binaries

Indexed keywords

ARCHIVAL DATA; CENTAURUS A; CHANDRA; FIELD POPULATIONS; FIELD SOURCES; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: GENERAL; LOW-MASS X-RAY BINARIES; LUMINOSITY FUNCTIONS; MILKY WAYS; POPULATION SYNTHESIS; QUANTITATIVE COMPARISON; SUB-POPULATIONS; UNIFORM COVERAGE; X RAY BINARIES; X-RAY BACKGROUND; X-RAY LUMINOSITY; X-RAY SOURCES; X-RAYS: BINARIES;

GALAXIES; POPULATION STATISTICS; STARS; X RAY OPTICS; X RAYS;

LUMINANCE;

EID: 80051965485     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116936     Document Type: Article

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