H-R Diagram for early type Magellanic Cloud members

Details H-R Diagram for early type Magellanic Cloud members H-R Diagram for early type Magellanic Cloud members

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..281n&link_type=abstract

In ESA 3rd European IUE Conf. p 281-282 (SEE N83-11889 02-88)

Computer Science

Early Stars, Hertzsprung-Russell Diagram, Magellanic Clouds, Giant Stars, Interstellar Extinction, Iue, Stellar Luminosity, Stellar Magnitude, Stellar Temperature, Supergiant Stars, Ultraviolet Spectra

Scientific paper

Low resolution UV spectra of a sample of Large Magellanic Cloud (LMC) early type members were obtained with the IUE. The sample includes 25 supergiants and 4 giants. Complementary visible data were obtained. The effective temperatures and bolometric magnitudes of these objects were determined by comparison with models. Results indicate that there is no significant difference between LMC and galactic stars.

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