The Environment of LBVs in M33

Details The Environment of LBVs in M33 The Environment of LBVs in M33

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..783...33b&link_type=abstract

THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP Conference Proceedings, Volume 783, pp. 33-36 (200

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Variable Stars, Galaxies, Star Formation, Stellar Photometry, Emission-Line Stars, Spiral Galaxies, Origin, Formation, Evolution, Age, And Star Formation, Hertzsprung-Russell, Color-Magnitude, And Color-Color Diagrams

Scientific paper

In this work we investigate the surroundings of LBVs in M33 using images from the NOAO Local Group Survey. PSF photometry has been performed in all filters and color-magnitude and color-color diagrams were produced for the full data set. We present a closer look on the known LBVs in M33 which are Var B, Var C, Var 2 and Var 83. Presented is an analysis of their stellar and gaseous environment in order to examine the possible connection to nearby associations. This is tried among other things by estimating the distance the star could have travelled since its formation. The motivaton for this is to investigate whether massive stars are built in associations with other maybe also massive stars or if they form as single stars.

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