UBVRI photometry in the field of NGC 2264

Details UBVRI photometry in the field of NGC 2264 UBVRI photometry in the field of NGC 2264

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.190..623m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 190, Feb. 1980, p. 623-630.

Astronomy and Astrophysics

Astronomy

32

Electrophotometry, Star Clusters, Ubv Spectra, Variable Stars, Visual Photometry, Carbon Stars, Chronology, Interstellar Extinction, Radial Velocity, Stellar Evolution, Stellar Magnitude, Stellar Spectra, T Tauri Stars

Scientific paper

The paper presents UBVRI photoelectric photometry for 70 stars in the field of NGC 2264. Attention is given to a comparison of these data with Walker's UBV photometry which indicates possible small light variations for a number of stars, and a significant change for W 90. It is reported that the (B-V, V-R) diagram clearly shows at least one T Tauri-like object and a possible carbon star, which is probably a background star. Finally, nearly 40 percent of the stars have variable velocities or probable variable velocities.

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