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Pulsations of the Oe Star ζ Ophiuchi from MOST Satellite Photometry and Ground-based Spectroscopy
- 1.0028560 - ASÚ 2006 RIV US eng J - Journal Article
Walker, G. A. H. - Kuschnig, R. - Matthews, J.M. - Reegen, P. - Kallinger, T. - Kambe, E. - Saio, H. - Harmanec, P. - Guenther, D.B. - Moffat, A.F.J. - Rucinski, S.M. - Sasselov, D. - Weiss, W.W. - Bohlender, D.A. - Božić, H. - Hashimoto, O. - Koubský, Pavel - Mann, R. - Ruždjak, D. - Škoda, Petr - Šlechta, Miroslav - Sudar, D. - Wolf, M.
Pulsations of the Oe Star ζ Ophiuchi from MOST Satellite Photometry and Ground-based Spectroscopy.
[Pulsace Oe hvězdy zeta Ophiuchi z fotometrie satelitu MOST a pozemské spektrospkopie.]
Astrophysical Journal. Roč. 623, č. 2 (2005), L145-L148. ISSN 0004-637X. E-ISSN 1538-4357
R&D Projects: GA AV ČR KSK2043105
Institutional research plan: CEZ:AV0Z1003909
Keywords : line profiles * emission-line stars * Be stars
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 6.308, year: 2005
Zeta Oph is the most rapidly rotating Be star. Simultaneous photometric and spectroscopic observation allows the determination of the plausible model of non-radial pulsations
Zeta Oph je nejrychleji rotující známá Be hvězda. Paralelní spektroskopie a fotometrie umožňuje vytvořit plausibilní model neradiálních pulsací.
Permanent Link: http://hdl.handle.net/11104/0118488
Number of the records: 1