High-mass X-ray binary SXP18.3 undergoes the longest type II outburst ever seen in the Small Magellanic Cloud

Monthly Notices of the Royal Astronomical Society

Volumn 392, Issue 1, 2009, Pages 361-366

  Schurch, M P E ^a   Coe, M J ^a   Galache, J L ^b   Corbet, R H D ^c   McGowan, K E ^a   McBride, V A ^a   Townsend, L J ^a   Udalski, A ^d   Haberl, F ^e  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

^d UNIVERSITY OF WARSAW   (Poland)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

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

Indexed keywords

STARS;

BE-X-RAYS:BINARIES; HIGH MASS X RAY BINARIES; MAGELLANIC CLOUDS; OPTICAL-; PULSE TIMING; SMALL MAGELLANIC CLOUDS; STARS: EMISSION-LINE BE; TYPE II; X-RAY TIMING EXPLORERS; X-RAYS: BINARIES;

GALAXIES;

EID: 57849147627     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14048.x     Document Type: Article

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