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Astronomy & Astrophysics manuscript no. reference2 c ESO 2009 June 29, 2009
 

Summary: Astronomy & Astrophysics manuscript no. reference2 c ESO 2009
June 29, 2009
The chemical abundance analysis of normal early A- and late
B-type stars
L. Fossati1, T. Ryabchikova1,2, S. Bagnulo3, E. Alecian4,5, J. Grunhut5, O. Kochukhov6, and G. Wade5
1
Institut f¨ur Astronomie, Universit¨at Wien, T¨urkenschanstrasse 17, 1180 Wien, Austria.
e-mail: fossati@astro.univie.ac.at,ryabchik@astro.univie.ac.at
2
Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya 48, 119017 Moscow, Russia.
e-mail: ryabchik@inasan.ru
3
Armagh Observatory, College Hill, Armagh BT61 9DG, Northern Ireland, UK.
e-mail: sba@arm.ac.uk
4
Observatoire de Paris-Meudon, LESIA, UMR 8111 du CNRS, 92195 Meudon Cedex, France.
e-mail: evelyne.alecian@obspm.fr
5
Physics Dept., Royal Military College of Canada, PO Box 17000, Station Forces, K7K 4B4, Kingston, Canada.
e-mail: Jason.Grunhut@rmc.ca,Gregg.Wade@rmc.ca

  

Source: Armagh Observatory

 

Collections: Physics