Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 9, N 8 (2009) |
ISSN 2221–0474 |
Received: 2.02.2009; accepted: 19.02.2009
(E-mail for contact: stephan.bakan@t-online.de)
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Remarks: |
While observing LL Aqr, the variability of GSC 05236-00391 was recognized. The presented
results are based on observations from 6 nights between 25 September 2008 and 10 January
2009, performed with a Schmidt-Newton 6" telescope and a Meade DSIProII
CCD camera, through a Schuler V filter. The comparison star was GSC 05236-00711;
GSC 05236-00492 was used as a check star. Our provisional analysis of this star in
the NSVS
(ROTSE-I) and ASAS-3 sky surveys
resulted in very similar light elements.
MinII = 13.71. |
Light Curve Finding Chart Data Source |