Ring nebulae around Wolf-Rayet stars in M33

Details Ring nebulae around Wolf-Rayet stars in M33 Ring nebulae around Wolf-Rayet stars in M33

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101.1659d&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, May 1991, p. 1659-1662, 1947-1951. NSERC-supported research.

Other

15

H Ii Regions, Nebulae, Spiral Galaxies, Wolf-Rayet Stars, H Alpha Line, Interstellar Matter, Milky Way Galaxy

Scientific paper

Results of a systematic search for H II ring nebulae surrounding Wolf-Rayet (WR) stars in M33 are presented. Eleven objects are found to be good candidates, while eight others are classified as possible WR ring nebulae. The WR rings in M33 are larger on average than their Galactic counterparts, but the H-alpha luminosity of most of them is comparable to the bright Galactic wind-blown bubbles. The rings are associated with WC as well as with WN stars.

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