Inferences from pulsational amplitudes and phases for multimodeδSct star FG Vir-Reference-Cited by-同舟云学术

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Inferences from pulsational amplitudes and phases for multimodeδSct star FG Vir

Published:2005-07-08 Issue:2 Volume:438 Page:653-660
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Daszyńska-Daszkiewicz J.,Dziembowski W. A.,Pamyatnykh A. A.,Breger M.,Zima W.,Houdek G.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20052902/pdf

Reference26 articles.

1. Low-temperature Rosseland opacities

2. Badnell, N. R., Bautista, M. A., Butler, K., et al. 2005, MNRAS, in press [arXiv:astro-ph/0410744]

3. Solar pulsational stability - III. Acoustical excitation by turbulent convection

4. New grids of ATLAS9 atmospheres

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1. Multimode δ Sct stars from the Zwicky Transient Facility Survey;The Astrophysical Journal Supplement Series;2024-06-28

2. Asteroseismology of double-mode radial δ Scuti stars: AE Ursae Majoris and RV Arietis;Monthly Notices of the Royal Astronomical Society;2023-09-13

3. Revisiting the δ Scuti star FG Virginis using Kepler K2 and TESS data;Frontiers in Astronomy and Space Sciences;2022-08-30

4. Asteroseismology of the double-radial mode δ Scuti star BP Pegasi;Monthly Notices of the Royal Astronomical Society;2022-03-10

5. Mode identification and seismic study of δ Scuti, the prototype of a class of pulsating stars;Monthly Notices of the Royal Astronomical Society;2021-05-11

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