Photometry of a Group of Stars in the Direction of NGC 1746/1750/1758

Details Photometry of a Group of Stars in the Direction of NGC 1746/1750/1758 Photometry of a Group of Stars in the Direction of NGC 1746/1750/1758

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pasp..122.1008l&link_type=abstract

Publications of the Astronomical Society of the Pacific, Volume 122, issue 895, pp.1008-1014

Astronomy and Astrophysics

Astronomy

Star Clusters And Associations

Scientific paper

UBV broadband photometry is reported for 19 stars in the direction of the Galactic (open) star clusters NGC 1746/1750/1758. Nine of these stars possess proper motions that point to the existence of a group centered at α=0504 and δ=+23°43.5. One known variable star, V1153 Tau, is recovered, and an emission-line star, HD 32318, is shown to be a variable star. RT Tau is reconfirmed to be constant in light.

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