Observational Evidence of the Evolutionary Enhancement of the Be Phenomenon

Details Observational Evidence of the Evolutionary Enhancement of the Be Phenomenon Observational Evidence of the Evolutionary Enhancement of the Be Phenomenon

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..363f&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

1

Scientific paper

Observational results obtained during the past few years support the existence of an evolutionary enhancement of the Be phenomenon along the B stars main sequence lifetime. In this paper we analyze recent related work, including: i/ the study of the frequency of Be stars in open clusters as a function of the cluster age; ii/the detailed analysis of the frequency of Be stars as a function of the spectral subtype in a few well studied young clusters; iii/ the determination of the evolutionary status of Be stars in the galactic field.

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