Optical follow-up of new Small Magellanic Cloud wing Be/X-ray binaries

Monthly Notices of the Royal Astronomical Society

Volumn 381, Issue 4, 2007, Pages 1561-1568

  Schurch, M P E ^a   Coe, M J ^a   McGowan, K E ^a   McBride, V A ^a   Buckley, D A H ^b   Galache, J L ^c   Corbet, R H D ^d   Still, M ^b   Vaisanen, P ^b   Kniazev, A ^b   Nordsieck, K ^b  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

Author keywords

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

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GALAXIES; X RAY SPECTROSCOPY;

BE STARS; BE-X-RAYS:BINARIES; CHANDRA; GROUND-BASED TELESCOPES; MAGELLANIC CLOUDS; OPTICAL FOLLOW-UP; OPTICAL-; SMALL MAGELLANIC CLOUDS; STARS: EMISSION-LINE BE; X-RAYS: BINARIES;

STARS;

EID: 35748932346     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12315.x     Document Type: Article

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