CALIBRATING CONVECTIVE PROPERTIES OF SOLAR-LIKE STARS IN THE KEPLER FIELD OF VIEW

• Type: Article in International Scientific Journal
• Date: 2012

Authors

Bonaca, A (Author) Other; Joel D Tanner (Author) Other; Sarbani Basu (Author) Other; William J Chaplin (Author) Other; Travis S Metcalfe (Author) Other; Monteiro, MPFG (Author) FCUP; Jerome Ballot (Author) Other; Timothy R Bedding (Author) Other; Alfio Bonanno (Author) Other; Anne Marie Broomhall (Author) Other; Hans Bruntt (Author) Other; Tiago L Campante (Author) Other; Jorgen Christensen Dalsgaard (Author) Other; Enrico Corsaro (Author) Other; Yvonne Elsworth (Author) Other; Rafael A Garcia (Author) Other; Saskia Hekker (Author) Other; Christoffer Karoff (Author) Other; Hans Kjeldsen (Author) Other; Savita Mathur (Author) Other; Clara Regulo (Author) Other; Ian Roxburgh (Author) Other; Dennis Stello (Author) Other; Regner Trampedach (Author) Other; Thomas Barclay (Author) Other; Christopher J Burke (Author) Other; Douglas A Caldwell (Author) Other

Journal

Title: Astrophysical Journal Letters

Vol. 755

Final page: L12

ISSN: 2041-8205

Publisher: American Astronomical Society

Indexing

ISI Web of Knowledge - 73 Citations

Scopus - 78 Citations

Scientific classification

FOS: Natural sciences > Physical sciences

CORDIS: Physical sciences > Astronomy

Other information

Authenticus ID: P-002-6Z7

DOI: 10.1088/2041-8205/755/1/l12

Abstract (EN): Stellar models generally use simple parameterizations to treat convection. The most widely used parameterization is the so-called mixing-length theory where the convective eddy sizes are described using a single number, alpha, the mixing-length parameter. This is a free parameter, and the general practice is to calibrate alpha using the known properties of the Sun and apply that to all stars. Using data from NASA's Kepler mission we show that using the solar-calibrated alpha is not always appropriate, and that in many cases it would lead to estimates of initial helium abundances that are lower than the primordial helium abundance. Kepler data allow us to calibrate alpha for many other stars and we show that for the sample of stars we have studied, the mixing-length parameter is generally lower than the solar value. We studied the correlation between alpha and stellar properties, and we find that alpha increases with metallicity. We therefore conclude that results obtained by fitting stellar models or by using population-synthesis models constructed with solar values of alpha are likely to have large systematic errors. Our results also confirm theoretical expectations that the mixing-length parameter should vary with stellar properties.

Language: English

Type (Professor's evaluation): Scientific