Long-term variability of the Be/X-ray binary a 0535 + 26 - I. Optical and UV spectroscopy

Monthly Notices of the Royal Astronomical Society

Volumn 294, Issue 1, 1998, Pages 165-176

  Clark, J S ^a   Tarasov, A E ^b   Steele, I A ^a,c   Coe, M J ^a   Roche, P ^d   Shrader, C ^e   Buckley, D A H ^f   Larionov, V ^g   Larionova, L ^g   Lyuty, V M ^b   Zaitseva, G V ^b   Grunsfeld, J ^e   Fabregat, J ^h   Parise, R ^e  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b CRIMEAN ASTROPHYSICAL OBSERVATORY   (Ukraine)

^c LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF SUSSEX   (United Kingdom)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

^f SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^g ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^h UNIVERSITY OF VALENCIA   (Spain)

Author keywords

Binaries: close; Pulsars: individual: A 0535 + 26 X rays: stars; Stars: emission line, Be

Indexed keywords

PHOTOMETRY; PULSARS; SPECTROSCOPIC ANALYSIS;

BE-X-RAYS:BINARIES; BINARIES: CLOSE; EQUIVALENT WIDTH; LONG-TERM VARIABILITY; OPTICAL-; PHOTOMETRICS; PULSAR: INDIVIDUAL: A 0535 + 26 - X-RAY: STAR; PULSARS:INDIVIDUAL; STARS: EMISSION-LINE BE; X-RAY:STARS;

ULTRAVIOLET SPECTROSCOPY;

EID: 0001723568     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01257.x     Document Type: Article

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