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Red giants seismology

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Conference object 01 Jan 2013Embargo end date: 01 Jan 2013Publisher:arXiv
Authors: Mosser, Benoît; Samadi, Davoud-Reza; Belkacem, Kevin;

doi: 10.48550/arxiv.1310.4748

arXiv: http://arxiv.org/abs/1310.4748

Red giants seismology

Abstract

The space-borne missions CoRoT and Kepler are indiscreet. With their asteroseismic programs, they tell us what is hidden deep inside the stars. Waves excited just below the stellar surface travel throughout the stellar interior and unveil many secrets: how old is the star, how big, how massive, how fast (or slow) its core is dancing. This paper intends to \emph{paparazze} the red giants according to the seismic pictures we have from their interiors.

SF2A 2013 conference

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Keywords

Astrophysics - Solar and Stellar Astrophysics, FOS: Physical sciences, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Solar and Stellar Astrophysics (astro-ph.SR)

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green