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Properties and nature of Be stars. 26. Long-term and orbital changes of zetaTauri
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SYSNO ASEP 0338396 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Properties and nature of Be stars. 26. Long-term and orbital changes of zetaTauri Author(s) Ruždjak, D. (HR)
Božić, H. (HR)
Harmanec, P. (CZ)
Fiřt, R. (DE)
Chadima, P. (CZ)
Bjorkman, K.S. (US)
Gies, D. R. (US)
Kaye, A.B. (US)
Koubský, Pavel (ASU-R) RID, ORCID
McDavid, D. (US)
Richardson, N. (US)
Sudar, D. (HR)
Šlechta, Miroslav (ASU-R) RID, ORCID
Wolf, M. (CZ)
Yang, S. (CA)Source Title Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 506, č. 3 (2009), s. 1319-1333Number of pages 15 s. Language eng - English Country FR - France Keywords early-type stars ; spectroscopic ; emission-line Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GA205/03/0788 GA ČR - Czech Science Foundation (CSF) GD205/08/H005 GA ČR - Czech Science Foundation (CSF) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000271514900024 DOI 10.1051/0004-6361/200810526 Annotation Our goal is to find the true timescales of its variability and confront them with the existing models related to various aspects of the Be phenomenon. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2010
Number of the records: 1