[Aavso-photometry] Variability of GSC 2362-2866

[Pertti Pääkkönen]

Dear fellows,

Let me introduce our observation of GSC 2362-2866 in Perseus, which was found 
to be a variable star during ITM's observation of (93)Minerva. The star 
appears to be a W UMa eclipsing binary with 7 hours period and variability 
between V=13.45...14.05. Results of 395 observations and analysis are 
collected in the page http://cc.joensuu.fi/seulaset/ccd/VAR2362-2866/
The discovery report is already submitted to IBVS. The observational data is 
not yet submitted to AAVSO.

Clear skies,

Pertti

-- 
Pertti Pääkkönen, PhD, Laboratory engineer
University of Joensuu, Department of Physics, Finland
Tel: +358 13 251 3238
Fax: +358 13 251 3290