The identification of the optical/IR counterpart to the ROSAT SMC X-ray transient RX J0117.6 - 7330

Monthly Notices of the Royal Astronomical Society

Volumn 293, Issue 1, 1998, Pages 43-48

  Coe, M J ^a   Buckley, D A H ^b   Charles, P A ^c   Southwell, K A ^c   Stevens, J B ^a  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^c UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Binaries: close; Infrared: stars; Magellanic Clouds; Pulsars: general; Stars: emission line, Be; X rays: stars

Indexed keywords

GALAXIES; PULSARS;

BINARIES: CLOSE; INFRARED: STAR; MAGELLANIC CLOUDS; MAGELLANIC CLOUDS-X-RAYS; OPTICAL-; PULSARS: GENERAL; SMALL MAGELLANIC CLOUDS; STARS: EMISSION-LINE BE; X-RAY TRANSIENTS; X-RAY:STARS;

ELECTROMAGNETIC WAVE EMISSION;

EID: 0002185773     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01111.x     Document Type: Article

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