Spectral types and UBV magnitudes of stars in the 30 Doradus complex

Details Spectral types and UBV magnitudes of stars in the 30 Doradus complex Spectral types and UBV magnitudes of stars in the 30 Doradus complex

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...92..729s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 92, no. 4, March 1992, p. 729-748.

Astronomy and Astrophysics

Astrophysics

37

O Stars, Stellar Magnitude, Stellar Spectra, Stellar Spectrophotometry, Ubv Spectra, Wolf-Rayet Stars, Carbon Stars, Charge Coupled Devices, Magellanic Clouds

Scientific paper

Photometric and spectroscopic observations are described for stars in four selected areas in the periphery of the 30 Doradus region. The areas are located at distances ranging from 7 to 20 arcmin from the central cluster. UBV magnitudes and spectral types for more than 250 stars are presented. A total of 70 new O stars is reported, most of which are located in the two inner regions. Photometric and spectroscopic data are given of the Wolf-Rayet stars in the surveyed fields. For WR stars in tight clusters, spatially resolved photometry is given. A carbon star is also identified.

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