Successful asteroseismology for a better characterization of the exoplanet HAT-P-7b

M. Oshagh, A. Grigahcène, O. Benomar, M. A. Dupret, M. J.P.F.G. Monteiro, R. Scuflaire, N. C. Santos

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

It is well known that asteroseismology is the unique technique permitting the study of the internal structure of pulsating stars using their pulsational frequencies, which is per se very important. It acquires an additional value when the star turns out to be a planet host. In this case, the asteroseismic study output may be a very important input for the study of the planetary system. With this in mind, we use the large time-span of the Kepler public data obtained for the star system HAT-P-7, first to perform an asteroseismic study of the pulsating star using Time-Dependent-Convection (TDC) models. Secondly, we make a revision of the planet properties in the light of the asteroseismic study.

Original languageEnglish (US)
Title of host publicationStellar Pulsations - Impact of New Instrumentation and New Insights
EditorsJ.C. Suarez, R. Garrido, J. Christensen-Dalsgaard, L.A. Balona
PublisherSpringer Netherlands
Pages227-230
Number of pages4
ISBN (Print)9783642296291
DOIs
StatePublished - 2013
Event20th Conference on Stellar Pulsations, 2011 - Granada, Spain
Duration: Sep 5 2011Sep 9 2011

Publication series

NameAstrophysics and Space Science Proceedings
Volume31
ISSN (Print)1570-6591
ISSN (Electronic)1570-6605

Other

Other20th Conference on Stellar Pulsations, 2011
CountrySpain
CityGranada
Period9/5/119/9/11

ASJC Scopus subject areas

  • Physics and Astronomy(all)
  • Computer Science Applications
  • Spectroscopy
  • Space and Planetary Science
  • Nuclear and High Energy Physics

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