Stellar winds from hot stars in the Magellanic Clouds

Details Stellar winds from hot stars in the Magellanic Clouds Stellar winds from hot stars in the Magellanic Clouds

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..413h&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Jan. 15, 1980, p. 413-420.

Astronomy and Astrophysics

Astrophysics

32

Hot Stars, Magellanic Clouds, Stellar Winds, Supergiant Stars, Astronomical Catalogs, B Stars, Early Stars, Milky Way Galaxy, O Stars, Stellar Mass Ejection, Stellar Spectra

Scientific paper

Spectrographic data have been obtained of O and B supergiants in the Magellanic Clouds at dispersions 12 and 25 A/mm in the blue and 25 and 50 A/mm in the red. Mass loss phenomena, line radial velocities, and line intensities have been measured on them and are compared with similar data on galactic stars. There appear to be some differences between the SMC, LMC, and the Galaxy in all these respects. Mass loss is clearly occurring in the Magellanic Cloud stars, and the SMC stars have particularly discrepant line intensities.

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