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Astronomy & Astrophysics manuscript no. Gpraesepe c ESO 2007 October 2, 2007
 

Summary: Astronomy & Astrophysics manuscript no. Gpraesepe c ESO 2007
October 2, 2007
Late stages of the evolution of A-type stars on the main sequence:
comparison between observed chemical abundances and diffusion
models for 8 Am stars of the Praesepe cluster
L. Fossati1, S. Bagnulo2, R. Monier3, S. A. Khan4, O. Kochukhov5, J. Landstreet4, G. Wade6, and W. Weiss1
1
Institut fur Astronomie, Universit¨at Wien, T¨urkenschanzstrasse 17, 1180 Wien, Austria.
e-mail: fossati@astro.univie.ac.at; weiss@astro.univie.ac.at
2
Armagh Observatory, College Hill, Armagh BT61 9DG, Northern Ireland. e-mail: sba@arm.ac.uk
3
Groupe de Recherches en Astronomie et Astrophysique du Languedoc UMR 5024, Universit´e Montpellier II, Place E. Bataillon,
34095 Montpellier, France. e-mail: Richard.Monier@graal.univ-montp2.fr
4
Department of Physics & Astronomy, University of Western Ontario, London, N6A 3K7, Ontario, Canada.
e-mail: skhan@astro.uwo.ca; jlandstr@astro.uwo.ca
5
Department of Astronomy and Space Physics, Uppsala University, 751 20, Uppsala, Sweden. e-mail: oleg@astro.uu.se
6

  

Source: Armagh Observatory

 

Collections: Physics