A Bayesian approach to scaling relations for amplitudes of solar-like oscillations in Kepler stars-Reference-Cited by-同舟云学术

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A Bayesian approach to scaling relations for amplitudes of solar-like oscillations in Kepler stars

Published:2013-02-07 Issue:3 Volume:430 Page:2313-2326
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Corsaro E.,Frohlich H.- E.,Bonanno A.,Huber D.,Bedding T. R.,Benomar O.,De Ridder J.,Stello D.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/430/3/2313/4933639/stt059.pdf

Reference61 articles.

1. Oscillation mode linewidths of main-sequence and subgiant stars observed byKepler

2. Visibilities and bolometric corrections for stellar oscillation modes observed byKepler

3. Amplitudes and lifetimes of solar-like oscillations observed by CoRoT

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