BVRI Photometry of the Eclipsing Spectroscopic Binary V1061 Cygni

Details BVRI Photometry of the Eclipsing Spectroscopic Binary V1061 Cygni BVRI Photometry of the Eclipsing Spectroscopic Binary V1061 Cygni

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...202.0805s&link_type=abstract

American Astronomical Society Meeting 202, #08.05; Bulletin of the American Astronomical Society, Vol. 35, p.708

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

A series of over 2000 images of the 9th magnitude eclipsing binary V1061 (HD235444, spectral type F8) was obtained during Autumn, 2002 using the 16-inch reflecting telescope of the Gettysburg College Observatory and a Photometrics 350 Camera equipped with a SITe 1024 x 1024 back-illuminated CCD chip. From the densely sampled BVRI light curves derived from these images, along with high-precision radial velocity data obtained at the Center for Astrophysics, we have computed a preliminary set of physical characteristics of the components of the V1061 Cygni system.

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