Spectral types in the open cluster NGC 6231

Details Spectral types in the open cluster NGC 6231 Spectral types in the open cluster NGC 6231

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92..323l&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, June 1980, p. 323-327.

Astronomy and Astrophysics

Astronomy

26

Open Clusters, Spectrum Analysis, Stellar Luminosity, Stellar Spectra, Classifications, Emission Spectra, Hertzsprung-Russell Diagram, Line Spectra, Stellar Evolution

Scientific paper

Accurate MK types for 26 of the brightest stars in the field of NGC 6231 have been determined. One emission-line star with a weak shell, one star with C III strong (already known), and four stars with double lines, (two of them previously known) have been found. Fitting the H-R diagram with the faint portion studied by Garrison and Schild (1979) provides an accurate H-R diagram for this young cluster.

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