UBV Photoelectric Photometry for Faint Stars in the Pleiades Cluster

Details UBV Photoelectric Photometry for Faint Stars in the Pleiades Cluster UBV Photoelectric Photometry for Faint Stars in the Pleiades Cluster

Apr 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967bott....4...79i&link_type=abstract

Boletín de los Observatorios de Tonantzintla y Tacubaya Vol. 4, pp. 79-83 (1967) (http://www.astroscu.unam.mx/bott/)

Astronomy and Astrophysics

Astronomy

19

Photometry, Galaxy: Open Clusters And Associations: Individual (Pleiades)

Scientific paper

Photoelectric photometry in the UBV system of Johnson and Morgan was carried out for 30 stars in the Pleiades Cluster. The main sequence between B-V=+0.6 and +0.8 was found to be very narrow, but from then on a broadening of the main sequence is apparent, even allowing for the larger observational errors. The observations were carried out at the 40-in telescope of the Tonantzintla Observatory.

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