UBV photometry of stars in the direction of three LMC X-ray sources

Details UBV photometry of stars in the direction of three LMC X-ray sources UBV photometry of stars in the direction of three LMC X-ray sources

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..769d&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Oct. 1975, p. 769-776.

Astronomy and Astrophysics

Astronomy

19

Magellanic Clouds, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, X Ray Stars, Error Analysis, Position (Location), Stellar Luminosity, X Ray Astronomy

Scientific paper

The results of UBV photometry of stars within or near the error boxes of LMC X-1, LMC X-2, and LMC X-3 are presented. The data on stars observed on several nights were analyzed for variability in their U, B, and V magnitudes. Suggestions are made concerning which stars around LMC X-1 and LMC X-3 are possibly variable and are promising candidates for the optical counterparts to these sources.

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