Preliminary Photometric Results for the 2003 Eclipse of Ee Cep

Details Preliminary Photometric Results for the 2003 Eclipse of Ee Cep Preliminary Photometric Results for the 2003 Eclipse of Ee Cep

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.296..445m&link_type=abstract

Astrophysics and Space Science, Volume 296, Issue 1-4, pp. 445-449

Astronomy and Astrophysics

Astrophysics

3

Binaries, Eclipsing-Stars, Individual, Ee Cep

Scientific paper

We report multicolour photometric observations of the 2003 eclipse of the long-period (5.6 yr) eclipsing binary EE Cep. Measurements were obtained with ten telescopes at eight observatories in four countries. In most cases, UBV(RI)C broad band filters have been used. The light curve shape shows that the obscuring body is an almost dark disk around a low-luminosity central object. However, variations of the colour indices during the eclipse indicate that the obscuring body emits a considerable amount of radiation in the near infrared.

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