Abundance analysis of targets for the COROT/MONS asteroseismology missions II. Abundance analysis of the COROT main targets

Autor(en)
H Bruntt, Ilfan F. Bikmaev, Claude Catala, Enrique Solano, Michel Gillon, Pierre Magain, C van 'T Veer-Menneret, Christian Stütz, Werner Wolfgang Weiss, Dominique Ballereau, Jean Claude Bouret, S Charpinet, T Hua, David Katz, Francois Lignieres, Theresa Rank-Lüftinger
Abstrakt

One of the goals of the ground-based support program for the COROT and MONS/RØMER satellite missions is to characterize suitable target stars for the part of the missions dedicated to asteroseismology. We present the detailed abundance analysis of nine of the potential COROT main targets using the semi-automatic software VWA. For two additional COROT targets we could not perform the analysis due to the high rotational velocity of these stars. For five stars with low rotational velocity we have also performed abundance analysis by a classical equivalent width method in order to test the reliability of the VWA software. The agreement between the different methods is good. We find that it is necessary to measure abundances extracted from each line relative to the abundances found from a spectrum of the Sun in order to remove systematic errors. We have constrained the global atmospheric parameters Teff log g, and [Fe/H] to within 70-100 K, 0.1-0.2 dex, and 0.1 dex for five stars which are slow rotators (? sin i <15 km s-1). For most of the stars we find good agreement with the parameters found from line depth ratios, Ha lines, Strošmgren indices, previous spectroscopic studies, and also log g determined from the HIPPARCOS parallaxes. For the fast rotators (v sin i > 60 km s-1) it is not possible to constrain the atmospheric parameters.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Copenhagen University Observatory, Kazan Federal University, Université de recherche Paris Sciences et Lettres, VILSPA - XMM Newton Science Operations Centre, Université de Liège, Université de Provence Aix-Marseille I, COROT Additional Program Working Group, Observatoire Midi-Pyrénées
Journal
Astronomy & Astrophysics
Band
425
Seiten
683-695
Anzahl der Seiten
13
ISSN
0004-6361
DOI
https://doi.org/10.1051/0004-6361:20040464
Publikationsdatum
2004
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/d38f7bb1-8410-42cd-8b58-a302defe1b7f