Photometrical research of open cluster NGC 7419

Details Photometrical research of open cluster NGC 7419 Photometrical research of open cluster NGC 7419

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ysc..conf...57b&link_type=abstract

12th Young Scientists' Conference on Astronomy and Space Physics, held in Kyiv, Ukraine, April 19-23, 2005, Eds.: Simon, A.; Gol

Physics

Space Physics

Scientific paper

The open cluster NGC 7419 is very interesting object. Pigulski and Kopacki pointed this cluster as richest for Be-stars abundance. We know the relationship between Be-phenomenon and Beta Chephei variability. In our research we try to find Beta Chephei variables in this cluster. Observational data were obtained in Kalinenkov Astronomical Observatory. We used telescope-reflector ZTS-702 (D=702mm, F=2.8m) with standard V-R-I light filters and radiation detector SBIG CCD ST-7.

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