Study of hubble space telescope counterparts to Chandra X-ray sources in the globular cluster M71

Astronomy and Astrophysics

Volumn 513, Issue 3, 2010, Pages

  Huang, R H H ^a   Becker, W ^a   Edmonds, P D ^b   Elsner, R F ^c   Heinke, C O ^d   Hsieh, B C ^e  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c NASA MARSHALL SPACE FLIGHT CENTER   (United States)

^d UNIVERSITY OF ALBERTA   (Canada)

^e INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

Author keywords

Globular clusters; Individual; M71 globular clusters; NGC 6838

Indexed keywords

APPROXIMATION THEORY; CAMERAS; ELECTRON SOURCES; OPTICAL PROPERTIES; OPTICAL TELESCOPES; SPACE TELESCOPES; X RAY APPARATUS;

ADVANCED CAMERA FOR SURVEYS; CATACLYSMIC VARIABLES; CHANDRA; COLLISION FREQUENCY; CORE DENSITIES; GLOBULAR CLUSTERS; HUBBLE SPACE TELESCOPES; MILLISECOND PULSARS; WIDE FIELD; X-RAY SOURCES;

X RAYS;

EID: 77951128685     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811245     Document Type: Article

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