R 136 - WN or O spectral characteristics

Details R 136 - WN or O spectral characteristics R 136 - WN or O spectral characteristics

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...113l..10v&link_type=abstract

Astronomy and Astrophysics, vol. 113, no. 2, Sept. 1982, p. L10-L12. Research supported by the Fonds de la Recherche Fondamenta

Astronomy and Astrophysics

Astronomy

10

Infrared Astronomy, O Stars, Stellar Spectra, Supermassive Stars, Wolf-Rayet Stars, Infrared Spectra, Magellanic Clouds, Near Infrared Radiation

Scientific paper

A near-IR spectroscopic study of R 136 finds no evidence of Wolf-Rayet characteristics, but presents clear similarities to the most luminous galactic O star, HD 93129. Additional agreement is noted between these findings and comments by Schmidt-Kaler and Feitzinger (1981), who find characteristics compatible with a hypothetical 02V or 01IF, as well as one of the alternatives proposed by Conti (1982).

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