The equatorial disc of the Be star X Persei

Monthly Notices of the Royal Astronomical Society

Volumn 296, Issue 4, 1998, Pages 785-799

  Telting, J H ^a,b   Waters, L B F M ^a   Roche, P ^c   Boogert, A C A ^d   Clark, J S ^e   De Martino, D ^f,g   Persi, P ^h  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^c UNIVERSITY OF SUSSEX   (United Kingdom)

^d UNIVERSITY OF GRONINGEN   (Netherlands)

^e UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^f VILSPA XMM Newton Science Operations Centre   (Spain)

^g INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^h CNR   (Italy)

Author keywords

Circumstellar matter; Infrared: stars; Stars: emission line, Be; Stars: individual: X per; Stars: mass loss; Ultraviolet: stars

Indexed keywords

BINARY ALLOYS; ELECTRON SCATTERING; GROWTH RATE; LUMINANCE; PHOTOMETRY;

BE STARS; CIRCUMSTELLAR MATTERS; EQUATORIAL DISKS; INFRARED: STAR; OPTICAL-; STAR: INDIVIDUAL: X PER; STARS: EMISSION-LINE BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MASS-LOSS; ULTRAVIOLET: STARS;

STARS;

EID: 1842636525     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01433.x     Document Type: Article

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