Abstract
We present the results of a spectral study of Galaxy No. 47 of the list [1]. We determine the equivalent widths of the lines for the compact part of the galaxy and the relative intensities for both the compact part and the halo. We estimate the mass of the galaxy from the inclination of the Hα line. We obtain the electron density and the mass of the gas component of the compact part of the galaxy.
Similar content being viewed by others
Literature cited
M. A. Kazaryan,Astrofizika,15, 5 (1979).
M. A. Kazaryan,Astrofizika,15, 193 (1979).
M. A. Kazaryan and E. S. Kazaryan,Astrofizika,16, 17 (1980).
M. A. Kazaryan and E. S. Kazaryan,Astrofizika,18, 512 (1982).
M. A. Kazaryan and E. S. Kazaryan,Astrofizika,19, 213 (1983).
M. A. Kazarian, E. Ye. Khachikian, and A. A. Yegiazarian,Astrophys. Space Sci.,82, 105 (1982).
M. A. Kazaryan,Astrofizika,20, 35 (1984).
M. A. Kazaryan,Astrofizika, in press (1995).
M. A. Kazaryan,Astrofizika,27, 399 (1987).
I. V. Nosov,Astron. Tsirk., No. 1050 (1979).
M. A. Kazaryan and V. S. Tamazyan,Astrofizika,36, 365 (1993).
M. A. Kazaryan and V. S. Tamazyan,Astron. Zh. Pis'ma,7, 276 (1981).
M. A. Kazaryan and E. S. Kazaryan,Astrofizika,33, 169 (1990).
Additional information
Translated fromAstrofizika, Vol. 38, No. 2, 1995.
Rights and permissions
About this article
Cite this article
Kazaryan, M.A., Karapetyan, E.L. Spectrophotometry of a Galaxy with UV-excess. Astrophysics 38, 133–136 (1995). https://doi.org/10.1007/BF02048587
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF02048587