Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...269..202c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 269, June 1, 1983, p. 202-211. Research supported by the American Astronomi
Astronomy and Astrophysics
Astrophysics
29
Interstellar Gas, Magellanic Clouds, Planetary Nebulae, Wolf-Rayet Stars, Astronomical Photography, Data Reduction, Kinematics, Milky Way Galaxy, Oxygen Spectra, Stellar Winds
Scientific paper
Echellograms with 4.6 A per mm dispersion have been obtained for four ring nebulae around Wolf-Rayet stars in the Large Magellanic Cloud (LMC): DEM 39, 231, 240, and 315. Their nature is analyzed and reported here. DEM 39 and DEM 315 are stellar wind blown bubbles, DEM 231 is probably an expanding hemisphere formed by the central star not necessarily during its W-R phase, and DEM 240 may have resulted from the interaction of stellar wind with a sheet of moving gas. A comparison of the bubbles blown by W-R stars in the Galaxy and the LMC is also made.
No associations
LandOfFree
Ring nebulae associated with Wolf-Rayet stars in the Large Magellanic Cloud. III - Kinematics of DEM 39, 231, 240, and 315 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Ring nebulae associated with Wolf-Rayet stars in the Large Magellanic Cloud. III - Kinematics of DEM 39, 231, 240, and 315, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ring nebulae associated with Wolf-Rayet stars in the Large Magellanic Cloud. III - Kinematics of DEM 39, 231, 240, and 315 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1504668