Optical photometry of the 1982-1984 eclipse of Epsilon Aurigae

Details Optical photometry of the 1982-1984 eclipse of Epsilon Aurigae Optical photometry of the 1982-1984 eclipse of Epsilon Aurigae

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985eepa.rept....7h&link_type=abstract

In NASA, Washington The 1982-1984 Eclipse of Epsilon Aurigae p 7-22 (SEE N86-12168 02-89)

Astronomy and Astrophysics

Astrophysics

3

Auriga Constellation, Eclipses, Eclipsing Binary Stars, Electrophotometry, Stellar Flares, Stellar Luminosity, Astrophysics, Brightness, Pulsed Radiation, Spectral Bands, Ultraviolet Photometry, Variable Stars

Scientific paper

From slightly before the 1982-1984 eclipse of Epsilon Aurigae to the present observers from around the world have been making photoelectric photometry observations of this star system. Over 2000 UBV observations have been reported as well as observations in the R, I, J, H, K, L, M, N, and Q bandpasses plus the y, b, v, and u bandpasses. Twenty nine observers from 9 countries submitted photometry data to the campaign. The data have shown many interesting features of the star system including a Cepheid-like pulsation, flare activity, mid-eclipse brightening, post egress brightening, plus other strange activity.

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