Properties and nature of Be stars: XXII. Long-term light and spectral variations of the new bright Be star HD 6226

Astronomy and Astrophysics

Volumn 416, Issue 2, 2004, Pages 669-676

  Bozic H ^a   Harmanec, P ^b,c   Yang, S ^d   Ziznovsky J ^e   Percy, J R ^f   Ruzdjak D ^a   Sudar, D ^a   Slechta M ^c   Skoda P ^c   Krpata, J ^b   Buil, C ^g  

^a UNIVERSITY OF ZAGREB   (Croatia)

^b CHARLES UNIVERSITY   (Czech Republic)

^c ASTRONOMICAL INSTITUTE   (Czech Republic)

^d UNIVERSITY OF VICTORIA   (Canada)

^e ASTRONOMICAL INSTITUTE   (Slovakia)

^f UNIVERSITY OF TORONTO   (Canada)

^g Assoc Utilisateurs Detecteurs E   (France)

Author keywords

Stars: binaries: spectroscopic; Stars: emission line, Be; Stars: individual: HD 6226

Indexed keywords

ABSORPTION; COLOR; CORRELATION METHODS; DAMPING; MATHEMATICAL TRANSFORMATIONS; PARAMETER ESTIMATION; PHOTOMETRY; PROBABILITY; ROTATION; SATELLITES; SPECTROSCOPIC ANALYSIS;

STARS: BINARIES: SPECTROSCOPIC; STARS: EMISSION-LINE; STARS: INDIVIDUAL: HD 6226;

ASTROPHYSICS;

EID: 12144291391     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031732     Document Type: Article

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