Home

About

Advanced Search

Browse by Discipline

Scientific Societies

E-print Alerts

Add E-prints

E-print Network
FAQHELPSITE MAPCONTACT US


  Advanced Search  

 
Mon. Not. R. Astron. Soc. 000, 113 (2010) Printed 4 January 2011 (MN LATEX style file v2.2) A detailed spectroscopic analysis of the open cluster NGC 5460
 

Summary: Mon. Not. R. Astron. Soc. 000, 1­13 (2010) Printed 4 January 2011 (MN LATEX style file v2.2)
A detailed spectroscopic analysis of the open cluster NGC 5460
L. Fossati,1,2
C.P. Folsom,3
S. Bagnulo,3
J.H. Grunhut,4
O. Kochukhov,5
J.D. Landstreet,3,6
C. Paladini,1
G.A. Wade,4
1Institut f¨ur Astronomie, Universit¨at Wien, T¨urkenschanzstrasse 17, 1180 Wien, Austria
2Department of Physics and Astronomy, Open University, Walton Hall, Milton Keynes MK7 6AA, UK
3Armagh Observatory, College Hill, Armagh BT61 9DG, Northern Ireland, UK
4Physics Dept., Royal Military College of Canada, PO Box 17000, Station Forces, K7K 4B4, Kingston, Canada
5Department of Physics and Astronomy, Uppsala University, 751 20, Uppsala, Sweden
6Department of Physics & Astronomy, University of Western Ontario, London, N6A 3K7, Ontario, Canada
ABSTRACT
Within the context of a large project aimed at studying early F-, A- and late B-type stars
we present the abundance analysis of the photospheres of 21 members of the open cluster
NGC 5460, an intermediate age cluster (log t 8.2) previously unstudied with spectroscopy.

  

Source: Armagh Observatory

 

Collections: Physics