Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...54..417f&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 54, Dec. 1983, p. 417-422. Research supported by the Swiss N
Astronomy and Astrophysics
Astrophysics
Astronomical Photometry, Cassiopeia Constellation, Galactic Structure, Interstellar Matter, Late Stars, Luminosity, Main Sequence Stars, Star Distribution
Scientific paper
The present investigation is concerned with a star field in Cassiopeia which is centered about 0.5 deg south of NGC 7654. The field has a size of approximately 0.28 square degrees, and it contains 1765 stars down to a limiting magnitude of G = 18.1 m. Steinlin (1961) had taken 15 RGU-plates (5 for each color) with the 48 in Palomar Schmidt telescope. The reddening, density, and luminosity functions have been determined according to the three-color photometric methods of the Basle Institute. A northern half of the star field studied coincides with an area investigated by Voroshilov et al. (1972).
Fenkart R.
Kandemir Gulcin
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