Photographic photometry of the primary galaxy of the VV242 system

Details Photographic photometry of the primary galaxy of the VV242 system Photographic photometry of the primary galaxy of the VV242 system

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984velen.......90r&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), Oct. 1984, p. 90-93. In Russian.

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Galactic Clusters, Spiral Galaxies, Ubv Spectra, Astronomical Photography, Brightness Distribution, Galactic Structure, Multispectral Photography

Scientific paper

Results are presented of the photographic UBV photometry of NGC 7253a, the primary galaxy of the interacting binary system VV242. Observations were made with the 2.6-meter telescope of the Biurakan Astrophysical Observatory; the scale of the photographs was 20 arcsec/mm. A detailed photometric study shows that NGC 7253a is a giant spiral of late type, perturbed by the secondary component of VV242.

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