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Photometric deprojection of edge-on galaxies

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Abstract

Photometric deprojection is used to determine the stellar-disk and bulge parameters for several edge-on galaxies from the FGC catalog. The assumption that the galaxies of our sample belonging to the fourth (i.e., lowest) surface-brightness class in the FGC are edge-on, low-surface-brightness (LSB) galaxies is considered.

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Authors and Affiliations

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

    D. V. Bizyaev

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  1. D. V. Bizyaev
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__________

Translated from Pis'ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 26, No. 4, 2000, pp. 266–272.

Original Russian Text Copyright © 2000 by Bizyaev.

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Bizyaev, D.V. Photometric deprojection of edge-on galaxies. Astron. Lett. 26, 219–224 (2000). https://doi.org/10.1134/1.20385

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  • DOI: https://doi.org/10.1134/1.20385

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