Optical identification of multiple faint X-ray sources in the globular cluster NGC 6752: Evidence for numerous cataclysmic variables

Astrophysical Journal

Volumn 569, Issue 1 I, 2002, Pages 405-417

  Pooley, David ^a   Lewin, Walter H G ^a   Homer, Lee ^b   Verbunt, Frank ^c   Anderson, Scott F ^b   Gaensler, Bryan M ^a,d   Margon, Bruce ^e   Miller, Jon M ^a   Fox, Derek W ^f   Kaspi, Victoria M ^a,g   Van der Klis, Michiel ^h  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF WASHINGTON   (United States)

^c UTRECHT UNIVERSITY   (Netherlands)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e STScI   (United States)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g MCGILL UNIVERSITY   (Canada)

^h UNIVERSITY OF AMSTERDAM   (Netherlands)

Author keywords

Binaries: close; Globular clusters: general; Globular clusters: individual (NGC 6752); Novae, cataclysmic variables; X rays: stars

Indexed keywords

EID: 0000118035     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/339210     Document Type: Article

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