Nonradial p-modes in the G9.5 giant ϵ Ophiuchi? Pulsation model fits to MOST photometry-Reference-Cited by-同舟云学术

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Nonradial p-modes in the G9.5 giant ϵ Ophiuchi? Pulsation model fits to MOST photometry

Published:2007-12-04 Issue:2 Volume:478 Page:497-505
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Kallinger T.,Guenther D. B.,Matthews J. M.,Weiss W. W.,Huber D.,Kuschnig R.,Moffat A. F. J.,Rucinski S. M.,Sasselov D.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20078171/pdf

Reference28 articles.

1. Low-temperature Rosseland opacities

2. Detection of solar-like oscillations in the red giant star ϵ Ophiuchi by MOST spacebased photometry

3. The observation and simulation of stochastically excited solar p modess

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