Please use this identifier to cite or link to this item: https://elar.urfu.ru/handle/10995/90326
Title: Extended ionized-gas structures in seyfert 2 galaxy Mrk 78
Authors: Kozlova, D. V.
Moiseev, A. V.
Smirnova, A. A.
Issue Date: 2020
Publisher: Astronomical Institute, Slovak Academy of Sciences
Citation: Kozlova, D. V. Extended ionized-gas structures in seyfert 2 galaxy Mrk 78 / D. V. Kozlova, A. V. Moiseev, A. A. Smirnova. — DOI 10.31577/caosp.2020.50.1.309 // Contributions of the Astronomical Observatory Skalnate Pleso. — 2020. — Vol. 1. — Iss. 50. — P. 309-317.
Abstract: The search and study of extended emission-line regions (EELRs) related to AGN in early-type galaxies is interesting to probe the history of nuclear ionization activity and also to understand the process of external gas accretion. In this work, we present observations of the EELR in Mrk 78 obtained at the 6-m Russian telescope using the long-slit and 3D spectroscopy methods. We show that ionized-gas clouds at 12-16 kpc projected distances from the nucleus are ionized by the AGN radiation. Also we have checked if the galaxy appearing in the optical images in the immediate neighbourhood of Mrk 78 near the external clouds is a dwarf companion or a part of a tidal structure. However, the spectrum of this galaxy, SDSS J074240.37+651021.4, obtained at the 6-m telescope corresponds to a distant background galaxy with z = 0.38. © 2020, Astronomical Institute, Slovak Academy of Sciences.
Keywords: GALAXIES: ACTIVE
GALAXIES: INDIVIDUAL: MRK 78
GALAXIES: INTERACTIONS
GALAXIES: ISM
GALAXIES: SEYFERT
URI: http://elar.urfu.ru/handle/10995/90326
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85079276358
WOS ID: 000508244000027
PURE ID: 12014174
ISSN: 1335-1842
DOI: 10.31577/caosp.2020.50.1.309
Sponsorship: Russian Science Foundation, RSF: 17-12-01335
Ministry of Science and Higher Education of the Russian Federation
Acknowledgements. This study was supported by the Russian Science Foundation, project no. 17-12-01335 ‘Ionized gas in galaxy discs and beyond the optical radius’ and based on the observations conducted with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences carried out with the financial support of the Ministry of Science and Higher Education of the Russian Federation. Authors are grateful to Victor Afanasiev for his interest to this work. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
RSCF project card: 17-12-01335
Appears in Collections:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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