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Analysis of the B and Be-star populations of the double cluster h and χ Persei

Published online by Cambridge University Press:  18 January 2010

Amber N. Marsh ,
M. Virginia McSwain  and
Thayne Currie
Amber N. Marsh
Affiliation:
Department of Physics, Lehigh University, Bethlehem, PA, USA email: anm506@lehigh.edu, mcswain@lehigh.edu
M. Virginia McSwain
Affiliation:
Department of Physics, Lehigh University, Bethlehem, PA, USA email: anm506@lehigh.edu, mcswain@lehigh.edu
Thayne Currie
Affiliation:
Harvard Smithsonian Center for Astrophysics, Cambridge, MA, USA email: tcurrie@cfa.harvard.edu
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Abstract

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We present blue optical spectra of 92 members of h and χ Per obtained with the WIYN telescope at Kitt Peak National Observatory. From these spectra, several stellar parameters were measured for the B-type stars, including v sin i, Teff, log gpolar, M∗, and R∗. Strömgren photometry was used to measure Teff and log gpolar for the Be stars. We also analyze photometric data of cluster members and discuss the near- to mid-infrared excesses of Be stars.

Keywords

open clusters and associations: individual (NGC 869, NGC 884)stars: emission-linestars: Be
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 462 - 465
Copyright
Copyright © International Astronomical Union 2010

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