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A photometric study of the peculiar galaxy UGC 4332

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Abstract

BVR c photometry of the galaxy UGC 4332 is presented. It is shown that its inclusion in a list of candidate galaxies with polar rings is erroneous. In reality, it is a spiral galaxy with a powerful bulge and a disturbed dust disk viewed edge-on.

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Authors and Affiliations

  1. Astronomical Institute, St. Petersburg State University, Bibliotechnaya pl. 2, Petrodvorets, 198904, Russia

    V. A. Yakovleva, V. A. Gagen-Torn & G. M. Karataeva

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  1. V. A. Yakovleva
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  2. V. A. Gagen-Torn
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  3. G. M. Karataeva
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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 77, No. 8, 2000, pp. 591–598.

Original Russian Text Copyright © 2000 by Yakovleva, Gagen-Torn, Karataeva.

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Yakovleva, V.A., Gagen-Torn, V.A. & Karataeva, G.M. A photometric study of the peculiar galaxy UGC 4332. Astron. Rep. 44, 523–529 (2000). https://doi.org/10.1134/1.1306353

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  • DOI: https://doi.org/10.1134/1.1306353

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