LBVs in M33: Their Environments and Ages

Details LBVs in M33: Their Environments and Ages LBVs in M33: Their Environments and Ages

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..245b&link_type=abstract

Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology ASP Conference Series, Vol. 353, Proceedings of the Confe

Computer Science

1

Scientific paper

We are investigating the surroundings of LBVs in M33, in order to better understand the LBV phase in different environments. We present an analysis of the stellar neighbours (association memberships) of known LBVs in M33. With a comparison with stellar evolution models we give estimates of the mass and age of the LBVs. At the same time also the gaseous environment, possible connections to nebulae, and the influences of the neighbouring stars are discussed.

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