A study of the young massive cluster N90 in the SMC

Details A study of the young massive cluster N90 in the SMC A study of the young massive cluster N90 in the SMC

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101..933h&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, March 1991, p. 933-936, 1115.

Astronomy and Astrophysics

Astronomy

10

Magellanic Clouds, Star Clusters, Stellar Evolution, Stellar Mass, B Stars, H Gamma Line, O Stars, Stellar Luminosity, Ultraviolet Spectra, Visible Spectrum

Scientific paper

Optical and UV spectra of O and B stars in the compact nebulous cluster Henize N90 in the SMC are presented. The brightest stars are of type O and B, although the optical and UV classifications used here do not at all agree closely. The spectra, effective temperatures, bolometric luminosities, extinction, stellar winds, and the evolutionary state of these stars are discussed. The fainter stars appear to be pre-main-sequence.

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