Photometry of LMC X-ray candidates

Details Photometry of LMC X-ray candidates Photometry of LMC X-ray candidates

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.172p..41w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 172, Sept. 1975, p. 41P-47P.

Astronomy and Astrophysics

Astronomy

20

Astronomical Photometry, Binary Stars, Magellanic Clouds, Ubv Spectra, Variable Stars, X Ray Sources, Eclipsing Binary Stars, Radio Sources (Astronomy), Tables (Data), Variance (Statistics), X Ray Stars

Scientific paper

Results are reported for UBV photometry of the candidate stars for three of the X-ray sources in the Large Magellanic Cloud (LMC X-1, LMC X-2, LMC X-3). Since none of these sources is a proven eclipsing X-ray binary and identification cannot be established by correlating X-ray and optical periods, the candidate stars were examined for variability. No statistically significant variations are found in the examined candidates for LMC X-1 (CPD -69 deg 476 and CPD -69 deg 474) and LMC X-2 (HDE 271213). However, the data suggest variability in the LMC X-3 candidate (LMC X-3/8).

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