Red supergiants in M33 galaxy

Details Red supergiants in M33 galaxy Red supergiants in M33 galaxy

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pobeo..73..257v&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 73, p. 257 - 263 (2002). In: Proceedings of the T

Astronomy and Astrophysics

Astronomy

Galaxies, Red Supergiants, Spatial Distribution, Stellar Groups

Scientific paper

In the present work the spatial distribution of the red supergiants in M33 galaxy is discussed. The observational data exhibit stellar groups of high stellar density. The smallest 60 groups with stellar density corresponding to signal-to-noise ratio S/N > 5 have a mean size of 8.1" (≍30 pc). They are real stellar associations in M33. The size of the largest stellar groups found in M33 is of about 200" (~0.8 kpc) and is typical for a stellar complex.

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