Optical and X-ray variability of two Small Magellanic Cloud X-ray binary pulsars - SXP46.6 and SXP6.85

Monthly Notices of the Royal Astronomical Society

Volumn 384, Issue 2, 2008, Pages 821-826

  McGowan, K E ^a   Coe, M J ^a   Schurch, M P E ^a   Corbet, R H D ^b   Galache, J L ^c   Udalski, A ^d  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY OF WARSAW   (Poland)

Author keywords

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

Indexed keywords

GALAXIES; OPTICAL CORRELATION; PULSARS;

BINARY PULSARS; CIRCUMSTELLAR DISKS; MAGELLANIC CLOUDS; OPTICAL DATA; OPTICAL-; SMALL MAGELLANIC CLOUDS; STARS: EMISSION-LINE BE; X RAY DATA; X-RAY VARIABILITY; X-RAYS: BINARIES;

ELECTROMAGNETIC WAVE EMISSION;

EID: 38849143233     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12762.x     Document Type: Article

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