A New LBV Candidate in M33

Details A New LBV Candidate in M33 A New LBV Candidate in M33

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..149b&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

1

Scientific paper

For a better understanding of the characteristics and evolution of massive stars in the LBV phase, which are rare (short lifetime) and hard to find, it is mandatory to obtain a sample as complete as possible. M33, being the closest face-on spiral galaxy, is an ideal target to search for (candidate) LBVs, and to extend the sample of LBVs known. Within our systematic search we report here our first LBV candidate.

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