Detailed Studies of Radiogalaxy Mrk1032-Reference-Cited by-同舟云学术

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Detailed Studies of Radiogalaxy Mrk1032

Published:2020 Issue: Volume: Page:341-343
ISSN:2579-2776
Container-title:Communications of the Byurakan Astrophysical Observatory
language:en
Short-container-title:ComBAO

Author:

Hakopian S. A.¹,Dodonov S. N.²,Andreasyan R. R.¹

Affiliation:

1. NAS RA V. Ambartsumian Byurakan Astrophysical Observatory (BAO), Armenia

2. Special Astrophysical Observatory (SAO), Russia

Abstract

The first results of the observations of Mrk1032, conducted with the 6-m telescope of SAO Russia, are given. It is shown, in particular, that a large complex of HII-regions, revealed by the integral-field spectroscopy, is the main source of UV radiation in the galaxy.

Publisher

NAS RA Byurakan Astrophysical Observatory after V. A. Ambartsumian

Subject

General Medicine,General Chemistry

Reference6 articles.

1. Denisiuk E. K., Lipovetskii V. A., 1984, Astrofizika, 20, 525D

2. Hakopian S. A., 2013, arXiv:1403.0127,

3. Maehara H., Inoue M., Takase B., et al. 1985, PASJ, 37, 451M

4. Markarian B. E., Lipovetskii V. A., Stepanian D. A., 1979, Astrofizika, 13, 397M

5. Sanamian V. A., Kandalian R. A., 1968, Astrofizika, 4, 129A

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