The Magellanic Bridge: Evidence for a population of X-ray binaries

Monthly Notices of the Royal Astronomical Society

Volumn 403, Issue 2, 2010, Pages 709-713

  McBride, V A ^a   Bird, A J ^a   Coe, M J ^a   Townsend, L J ^a   Corbet, R H D ^b,c   Haberl, F ^d  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Binaries: general; Magellanic Clouds

Indexed keywords

GALAXIES;

BINARIES:GENERAL; ENERGY RANGES; HARD X-RAY SOURCES; HIGH MASS X RAY BINARIES; MAGELLANIC CLOUDS; OPTICAL-; SMALL MAGELLANIC CLOUDS; SPECTRAL CHARACTERISTICS; TIMING CHARACTERISTICS; X-RAYS: BINARIES;

STARS;

EID: 77952568076     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.16178.x     Document Type: Article

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