A spectroscopic analysis of B-stars in the SMC cluster NGC 330

Details A spectroscopic analysis of B-stars in the SMC cluster NGC 330 A spectroscopic analysis of B-stars in the SMC cluster NGC 330

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...66..169l&link_type=abstract

Space Science Reviews, Volume 66, Issue 1-4, pp. 169-172

Computer Science

14

Ngc330, B-Stars, Abundances, Evolution

Scientific paper

Medium resolution (2A/px) but high s/n spectra of approximately twenty of the brightest blue stars in the young open cluster NGC 330 in the SMC have been analyzed in order to determine their atmospheric parameters and the evolutionary status. Stellar parameters are determined by comparison with LTE and NLTE model atmosphere calculations and an HR diagram constructed. Luminosities of the sample stars lie in the range 4.0

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