CCD photometry in the fields of six eclipsing binaries in the Large and Small Magellanic Clouds. I - Light curves of the binaries - Standard V, B-V data and variability study for 161 selected stars in the fields

Details CCD photometry in the fields of six eclipsing binaries in the Large and Small Magellanic Clouds. I - Light curves of the binaries - Standard V, B-V data and variability study for 161 selected stars in the fields CCD photometry in the fields of six eclipsing binaries in the Large and Small Magellanic Clouds. I - Light curves of the binaries - Standard V, B-V data and variability study for 161 selected stars in the fields

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74..331j&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 2, Aug. 1988, p. 331-350. Research supported by the

Astronomy and Astrophysics

Astrophysics

18

Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Magellanic Clouds, Ubv Spectra, Variability, Charge Coupled Devices, Mass To Light Ratios, Precision

Scientific paper

CCD light curves with a precision of about 0m01 have been observed for six eclipsing binaries in the Large and Small Magellanic Clouds. These data allow the determination of accurate photometric elements, and results from the photometric analyses will be published separately. As a useful spin-off, standard V, B-V data for 161 selected stars close to the binaries are presented, and possible variables have been identified. For a few objects additional photoelectric uvby photometry is given.

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