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Название: Extended ionized-gas structures in seyfert 2 galaxy Mrk 78
Авторы: Kozlova, D. V.
Moiseev, A. V.
Smirnova, A. A.
Дата публикации: 2020
Издатель: Astronomical Institute, Slovak Academy of Sciences
Библиографическое описание: 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.
Аннотация: 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.
Ключевые слова: GALAXIES: ACTIVE
GALAXIES: INDIVIDUAL: MRK 78
GALAXIES: INTERACTIONS
GALAXIES: ISM
GALAXIES: SEYFERT
URI: http://elar.urfu.ru/handle/10995/90326
Условия доступа: info:eu-repo/semantics/openAccess
Идентификатор SCOPUS: 85079276358
Идентификатор WOS: 000508244000027
Идентификатор PURE: 12014174
ISSN: 1335-1842
DOI: 10.31577/caosp.2020.50.1.309
Сведения о поддержке: 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.
Карточка проекта РНФ: 17-12-01335
Располагается в коллекциях:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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