Variations in the brightness and polarization of W Cep

Details Variations in the brightness and polarization of W Cep Variations in the brightness and polarization of W Cep

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap.....49..164p&link_type=abstract

Astrophysics, Volume 49, Issue 2, pp.164-172

Astronomy and Astrophysics

Astrophysics

Stars, Photometry, Polarization-Individual, W Cep

Scientific paper

The hypothesis that W Cep has an eclipsing variability is discussed on the basis of our photometric and polarimetric observations of it from 1983-2003. Here we attempt to use our observations of W Cep to construct an average light curve, after separating out the slow variation, with the elements JDmin=2448105d+2090d. A strong variability is found from period to period at phases of 0.1-0.3 that may be caused by a variable flow of matter between the components.

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