Reference : Assessing the accuracy of the surface gravity determination in late-type stars with sola...
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/108389
Assessing the accuracy of the surface gravity determination in late-type stars with solar-like pulsators
English
Morel, Thierry mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE)]
Miglio, Andrea mailto [University of Birmingham > > > >]
1-Jan-2012
Monthly Notices of the Royal Astronomical Society
Blackwell Publishing
419
L34-L38
Yes (verified by ORBi)
International
0035-8711
Oxford
United Kingdom
[en] asteroseismology ; stars: fundamental parameters ; stars: late-type
[en] The frequency of maximum oscillation power measured in dwarfs and giants exhibiting solar-like pulsations provides a precise, and potentially accurate, inference of the stellar surface gravity. An extensive comparison for about 40 well-studied pulsating stars with gravities derived using classical methods (ionization balance, pressure-sensitive spectral features or location with respect to evolutionary tracks) supports the validity of this technique and reveals an overall remarkable agreement with mean differences not exceeding 0.05 dex (although with a dispersion of up to ˜0.2 dex). It is argued that interpolation in theoretical isochrones may be the most precise way of estimating the gravity by traditional means in nearby dwarfs. Attention is drawn to the usefulness of seismic targets as benchmarks in the context of large-scale surveys.
http://hdl.handle.net/2268/108389
10.1111/j.1745-3933.2011.01172.x
http://adsabs.harvard.edu/abs/2012MNRAS.419L..34M
http://de.arxiv.org/abs/1110.2036

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