The first Byurakan spectral sky survey. Investigations of stars of late M and C spectral classes

Details The first Byurakan spectral sky survey. Investigations of stars of late M and C spectral classes The first Byurakan spectral sky survey. Investigations of stars of late M and C spectral classes

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap.....38..300g&link_type=abstract

Astrophysics, Volume 38, Issue 4, pp.300-302

Astronomy and Astrophysics

Astrophysics

Scientific paper

The results of investigations of new faint M and C type stars discovered on the plates of the First Byurakan Spectral Sky Survey are reported. Among 161 newly discovered stars, 98 are identified with unknown IRAS point sources. It is probable that the majority of new M stars are Mirids according to their distributions on the IRAS color—color diagram. For J stars, a correlation between EW(C2 + CN) and EW(C2(0,1)) is found.

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