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30 Doradus: the stellar content and IMF

Published online by Cambridge University Press:  07 August 2017

Joel Wm. Parker
Joel Wm. Parker*
Affiliation:
CASA, Campus Box 389 University of Colorado Boulder, CO 80309-0389 USA

Extract

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I have UBV photometry for roughly 1500 stars and BV photometry for an additional 900 stars in the 30 Doradus region as a part of my thesis work. Spectra and spectral classifications for over 200 stars have been obtained (by me and various other sources) for most of the early stars in the region. The reductions and classifications are nearly complete. It should be noted that the OB associations of 30 Doradus present unique problems in the analysis of the stellar contents due to the extreme crowding and highly variable nebulosity and reddening.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 467
Copyright
Copyright © Kluwer 

References

Parker, J. Wm., Garmany, C.D., Massey, P., and Walborn, N.R. 1991, AJ, submitted.Google Scholar
Parker, J. Wm. and Walborn, N.R. 1991, ApJL, submitted.Google Scholar