[Previous] | [Session 8] | [Next]
H. A. Sheets, L.A. Marschall (Gettysburg College), G. Torres (Harvard-Smithsonian Center for Astrophysics)
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.
If you would like more information about this abstract, please follow the link to http://www.gettysburg.edu/academics/physics/clea/obshome.html. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
[Previous] | [Session 8] | [Next]
Bulletin of the American Astronomical Society, 35 #3
© 2003. The American Astronomical Soceity.