Spectral types in Gurzadyan's clustering in Auriga

Details Spectral types in Gurzadyan's clustering in Auriga Spectral types in Gurzadyan's clustering in Auriga

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90..555a&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, Oct.-Nov. 1978, p. 555, 556.

Astronomy and Astrophysics

Astronomy

Auriga Constellation, Star Clusters, Stellar Spectra, A Stars, Astrometry, B Stars, Early Stars

Scientific paper

Spectral types of the 11 brightest stars in Gurzadyan's (1974) clustering confirm that most of these are B stars. The conclusions of Heiser et al. (1978) are confirmed that there are several groups present: (1) a distant group at 1100 pc with 0.23 mag reddening and three evolved stars; (2) an intermediate group at 630 pc with 0.06 mag reddening and lying mostly northeast of the distant group but with some overlap; and (3) three foreground Am stars at 250-500 pc.

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