The super-soft source XMMU J052016.0-692505 in the LMC: A likely white dwarf Be/X-ray binary

Astronomy and Astrophysics

Volumn 458, Issue 1, 2006, Pages 285-292

  Kahabka, P ^a   Haberl, F ^a   Payne, J L ^b   Filipovic, M D ^c  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b JAMES COOK UNIVERSITY   (Australia)

^c UNIVERSITY OF WESTERN SYDNEY   (Australia)

Author keywords

Magellanic Clouds; Stars: emission line, Be; Stars: general; X rays: binaries; X rays: stars

Indexed keywords

BOLOMETERS; LIGHT SCATTERING; OPTICAL PROPERTIES; ORBITS; RADIO TELESCOPES; SPECTRUM ANALYSIS; X RAYS;

MAGELLANIC CLOUDS; STARS: EMISSION-LINE, BE; STARS: GENERAL; X-RAYS: BINARIES; X-RAYS: STARS;

GALAXIES;

EID: 33750264056     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065490     Document Type: Article

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