Preliminary abundances in three cool supergiants of the SMC

Details Preliminary abundances in three cool supergiants of the SMC Preliminary abundances in three cool supergiants of the SMC

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987msngr..48...37s&link_type=abstract

ESO Messenger (ISSN 0722-6691), June 1987, v. 48, p. 37-40.

Physics

2

Abundance, Cool Stars, Molecular Clouds, Stellar Spectrophotometry, Supergiant Stars, Dwarf Stars, Iron, Line Spectra, Metallicity

Scientific paper

Preliminary results for three field stars observed in the SMC are presented. The curve of growth of iron in the star AZVI 197 is shown. It is found that the metallicities of all the young supergiants in the SMC coincide, within determination errors, with the 'metallicities' (i.e., oxygen abundances) of young gaseous objects such as H II regions and planetary nebulae.

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