Reference : Solar-like pulsating stars as distance indicators: G-K giants in the CoRoT and Kepler fi...
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/130355
Solar-like pulsating stars as distance indicators: G-K giants in the CoRoT and Kepler fields
English
Miglio, A. [School of Physics and Astronomy, University of Birmingham, UK;]
Morel, Thierry [Université de Liège - ULg > > GAPHE : Astrophysique observationnelle (sol et espace) >]
Barbieri, M. [Observatoire de la Côte d'Azur, Nice, France]
Mosser, B. [LESIA, Observatoire de Paris, France]
Girardi, L. [INAF, Osservatorio Astronomico di Padova]
Montalban Iglesias, Josefa mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
Valentini, Marica [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
1-Feb-2012
European Physical Journal Web of Conferences
05012
No
International
Assembling the Puzzle of the Milky Way,Le Grand-Bornand, France, Edited by C. Reylé; A. Robin; M. Schultheis
Apr. 17-22, 2011
[en] The detection of radial and non-radial solar-like oscillations in thousands of G-K giants with CoRoT and Kepler is paving the road for detailed studies of stellar populations in the Galaxy. The available average seismic constraints allow a precise and largely model-independent determination of stellar radii (hence distances) and masses. We here briefly report on the distance determination of thousands of giants in the CoRoT and Kepler fields of view.
http://hdl.handle.net/2268/130355
10.1051/epjconf/20121905012
http://adsabs.harvard.edu/abs/2012EPJWC..1905012M
http://de.arxiv.org/abs/1111.4366
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