Hydrodynamic models for β Cephei variables I. BW Vulpeculae revisited

Astronomy and Astrophysics

Volumn 426, Issue 2, 2004, Pages 687-693

  Fokin, A ^a,b,d   Mathias, Ph ^b   Chapellier, E ^b   Gillet, D ^c   Nardetto, N ^b  

^a INSTITUTE OF ASTRONOMY   (Russian Federation)

^b UNIVERSITÉ CÔTE D'AZUR   (France)

^c CNRS   (France)

^d Isaak Newton Institute   (Russian Federation)

Author keywords

Line: profiles; Stars: individuals: BW Vulpeculae; Stars: oscillations; Stars: variables: general

Indexed keywords

BOLOMETERS; DAMPING; KINETIC ENERGY; LIGHT ABSORPTION; MATHEMATICAL MODELS; OSCILLATIONS; PHOTOMETRY; SIGNAL TO NOISE RATIO;

BW VULPECULAE; INDIVIDUALS; STARS; VARIABLES;

HYDRODYNAMICS;

EID: 8344225247     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040418     Document Type: Article

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