Distribution of WR stars in 2 nearby galaxies (Leloudas+, 2010)

Details Distribution of WR stars in 2 nearby galaxies (Leloudas+, 2010) Distribution of WR stars in 2 nearby galaxies (Leloudas+, 2010)

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35189029l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/518/A29. Originally published in: 2010A&A...518A..29L

Computer Science

Galaxies: Nearby, Stars: Variable

Scientific paper

We derived the relative surface brightness (fractional flux) at the locations of WR stars and compared with similar results for LGRBs and SNe. We examined two nearby galaxies, M 83 and NGC 1313, for which a comprehensive study of the WR population exists. These two galaxies contain a sufficiently large number of WR stars and sample different metallicities. To enable the comparison, the images of the galaxies were processed to make them appear as they would look at a higher redshift. The robustness of our results against several sources of uncertainty was investigated with the aid of Monte Carlo simulations.
(1 data file).

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