The binary period and outburst behaviour of the Small Magellanic Cloud X-ray binary pulsar system SXP504

Monthly Notices of the Royal Astronomical Society

Volumn 361, Issue 2, 2005, Pages 743-747

  Edge, W R T ^a   Coe, M J ^a   Galache, J L ^a   McBride, V A ^a   Corbet, R H D ^b,c   Okazaki, A T ^d   Laycock, S ^e   Markwardt, C B ^b,f   Marshall, F E ^b   Udalski, A ^g  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

^d HOKKAI GAKUEN UNIVERSITY   (Japan)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f UNIVERSITY OF MARYLAND   (United States)

^g UNIVERSITY OF WARSAW   (Poland)

Author keywords

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

Indexed keywords

GALAXIES;

BINARY PULSARS; CHANDRA; MAGELLANIC CLOUDS; MAGELLANIC CLOUDS-X-RAYS; OPTICAL-; PULSE PERIOD; SMALL MAGELLANIC CLOUDS; STARS: EMISSION-LINE BE; X-RAY SOURCES; X-RAYS: BINARIES;

PULSARS;

EID: 23444447655     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09205.x     Document Type: Article

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