UBV Monitoring of EPS Aurigae(i)

Details UBV Monitoring of EPS Aurigae(i) UBV Monitoring of EPS Aurigae(i)

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jass....5...53n&link_type=abstract

Journal of Astronomy and Space Science, vol. 5, no. 1, p. 53-56.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

UBV photometric monitoring of Eps Aurigae has been made at Yonsei University Observatory since the 1982-1984 eclipse. Among observations made in four seasons (1984-5, 1985-6, 1986-7, 1987-8) after the 1982-84 eclipse ended the observations of the latest season are presented. Standardized UBV light curves of Eps Aur exhibit a light variation in a semi-regular fashion with the amplitudes of 0.12, 0.19, and 0.29 for V, B, and U, respectively. Durations of this light variation may show a color dependency with the mean vale of about 78 days whose minimum light on near JD2447118.

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