Inferences from pulsational amplitudes and phases for multimode δ Sct star FG Vir

Astronomy and Astrophysics

Volumn 438, Issue 2, 2005, Pages 653-660

  Daszynska Daszkiewicz J ^a,b   Dziembowski, W A ^b,c   Pamyatnykh, A A ^b,d,e   Breger, M ^e   Zima, W ^e   Houdek, G ^f  

^a UNIVERSITY OF WROC AW   (Poland)

^b NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^c UNIVERSITY OF WARSAW   (Poland)

^d INSTITUTE OF ASTRONOMY   (Russian Federation)

^e UNIVERSITY OF VIENNA   (Austria)

^f UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

Scuti; Convection; Stars: fundamental parameters; Stars: oscillations

Indexed keywords

BOLOMETERS; DATA REDUCTION; HEAT CONVECTION; OSCILLATIONS; PROBABILITY; SPECTROSCOPIC ANALYSIS;

Δ SCUTI; PULSATION AMPLITUDES; STARS: FUNDAMENTAL PARAMETERS; STARS: OSCILLATIONS;

ASTROPHYSICS;

EID: 23244444202     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20052902     Document Type: Article

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