Photometry of the 'ultraviolet' stellar group in Auriga

Details Photometry of the 'ultraviolet' stellar group in Auriga Photometry of the 'ultraviolet' stellar group in Auriga

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90..105h&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, Feb.-Mar. 1978, p. 105-107. Research supported by the Vanderbilt Un

Astronomy and Astrophysics

Astronomy

1

Star Clusters, Stellar Spectrophotometry, Ubv Spectra, Ultraviolet Astronomy, Colorimetry, Main Sequence Stars, Stellar Evolution, Stellar Luminosity

Scientific paper

Ultraviolet stellar spectra obtained from a space observatory have suggested the probable existence of a small cluster of early-type stars in the constellation of Auriga. UBV and uvby photometry of these stars indicate that this small group apparently contains two subgroups at somewhat different distances and with distinctly different amounts of interstellar reddening. Two or three luminous stars may be part of the more distant subgroup.

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