CAOSP abstracts, Volume: 43, No.: 3, year: 2014

Abstract: V1010 Oph is a relatively bright near contact binary. We present a new study including four-colour photometry and a model of the system. The uniqueness of our study is in the using of only a centimetre-class telescope with a CCD camera. We show that such small, cheap equipment seems to be very helpful in the investigation of bright variable stars.

Full text version of this article in PostScript (600dpi) format compressed by gzip; or in PDF.

Back to:
CAOSP Vol. 43 No. 3 index
CAOSP archive main index
CAOSP main page
Astronomical Institute home page
Valid XHTML 1.0! Valid CSS!

Last update: April 17, 2014