Non-radially pulsating Be stars

Rivinius, Th.; Baade, D.; Štefl, S.

doi:10.1051/0004-6361:20031285

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Non-radially pulsating Be stars

Author(s): Th. Rivinius , D. Baade , S. Štefl

Publication date (Electronic): November 17 2003

Journal: Astronomy & Astrophysics

Publisher: EDP Sciences

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Statistical analysis of intrinsic polarization, IR excess and projected rotational velocity distributions of classical Be stars

R. Yudin (2001)

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Application of BEM (boundary element method)‐based acoustic holography to radiation analysis of sound sources with arbitrarily shaped geometries

Mingsian Bai (1992)

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A Study of π Aquarii during a Quasi‐normal Star Phase: Refined Fundamental Parameters and Evidence for Binarity

Karen Bjorkman, Anatoly Miroshnichenko, David A. McDavid … (2002)

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Author and article information

Journal

Title: Astronomy & Astrophysics

Abbreviated Title: A&A

Publisher: EDP Sciences

ISSN (Print): 0004-6361

ISSN (Electronic): 1432-0746

Publication date Created: November 2003

Publication date (Electronic): November 17 2003

Publication date (Print): November 2003

Volume: 411

Issue: 2

Pages: 229-247

Article

DOI: 10.1051/0004-6361:20031285

SO-VID: 77c959ad-4716-4d1a-8bbe-4010486e4d05

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Non-radially pulsating Be stars

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Most cited references 27

Statistical analysis of intrinsic polarization, IR excess and projected rotational velocity distributions of classical Be stars

Application of BEM (boundary element method)‐based acoustic holography to radiation analysis of sound sources with arbitrarily shaped geometries

A Study of π Aquarii during a Quasi‐normal Star Phase: Refined Fundamental Parameters and Evidence for Binarity

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