Spectral morphology in the open cluster NGC 2287

Details Spectral morphology in the open cluster NGC 2287 Spectral morphology in the open cluster NGC 2287

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..636l&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Oct.-Nov. 1979, p. 636-638. Research supported by the Comision de I

Astronomy and Astrophysics

Astronomy

16

Classifications, Open Clusters, Stellar Spectra, A Stars, B Stars, Binary Stars, K Lines, Magnetic Stars, Metallic Stars

Scientific paper

Spectral classifications in NGC 2287 have revealed the presence of an
He-weak star, three Hg-Mn stars, one star with a weak K line, one cool
Ap star and one star with a composite spectrum. Spectroscopic evidence
determined eight double-line binaries as well as five suspected
double-line binaries.

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