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BVRI CCD photometry of the peculiar galaxies NGC 5605 and NGC 5665

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Abstract

The paper presents the results of BVRI CCD photometry of the late-type peculiar galaxies NGC 5605 and NGC 5665 obtained on the 1.5-m telescope of the Ma\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\)danak Observatory (Uzbekistan). Regions of star formation are identified and studied. The compositions of the stellar populations in various regions of NGC 5605 and NGC 5665 are estimated using two-color diagrams. The ages of blue condensations (stellar aggregates) in the spiral arms of the galaxies are determined. It is concluded that NGC 5665 underwent an interaction with another galaxy 5×108 yr ago.

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Authors and Affiliations

  1. Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119899, Russia

    B. P. Artamonov, Yu. Yu. Badan & A. S. Gusev

  2. Institute of Solid-State Physics, Russian Academy of Sciences, Chernogolovka, Moscow oblast, 142432, Russia

    A. S. Gusev

Authors
  1. B. P. Artamonov
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  2. Yu. Yu. Badan
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  3. A. S. Gusev
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__________

Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 77, No. 9, 2000, pp. 643–653.

Original Russian Text Copyright © 2000 by Artamonov, Badan, Gusev.

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Artamonov, B.P., Badan, Y.Y. & Gusev, A.S. BVRI CCD photometry of the peculiar galaxies NGC 5605 and NGC 5665. Astron. Rep. 44, 569–578 (2000). https://doi.org/10.1134/1.1307552

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  • DOI: https://doi.org/10.1134/1.1307552

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