Chemical abundances in Seyfert galaxies -- V. The discovery of shocked emission outside the AGN ionization axis
| Autor: | Guillermo F. Hägele, Angela Krabbe, I. C. Freitas, Mónica V. Cardaci, Nadia L. Zakamska, D. Ruschel-Dutra, Anna Feltre, Mark Kojo Armah, Thaisa Storchi-Bergmann, Rogemar A. Riffel, O. L. Dors, Enrique Pérez-Montero |
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| Přispěvatelé: | Ministerio de Economía y Competitividad (España), European Commission |
| Jazyk: | angličtina |
| Rok vydání: | 2020 |
| Předmět: |
Gemini Observatory
Physics Ciencias Astronómicas Seyfert [Galaxies] Galaxies: Seyfert active [Galaxies] Galaxies: abundances Astrophysics::High Energy Astrophysical Phenomena FOS: Physical sciences Astronomy abundances [Galaxies] Astronomy and Astrophysics Galaxies: active Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics - Astrophysics of Galaxies Galaxy Galaxies: ISM Space and Planetary Science Research council Astrophysics of Galaxies (astro-ph.GA) ISM [Galaxies] Space Science Astrophysics::Galaxy Astrophysics |
| Zdroj: | Digital.CSIC. Repositorio Institucional del CSIC instname |
| Popis: | We present maps for the electron temperature in the inner kpc of three luminous Seyfert galaxies: Mrk 79, Mrk 348, and Mrk 607 obtained from Gemini Multi-Object Spectrograph-integral field unit observations at spatial resolutions of ∼110–280 pc. We study the distributions of electron temperature in active galaxies and find temperatures varying in the range from ∼8000 to ≳30000K. Shocks due to gas outflows play an important role in the observed temperature distributions of Mrk 79 and Mrk 348, while standard photoionization models reproduce the derived temperature values for Mrk 607. In Mrk 79 and Mrk 348, we find direct evidence for shock ionization with overall orientation orthogonal to the ionization axis, where shocks can be easily observed as the active galactic nuclei radiation field is shielded by the nuclear dusty torus. This also indicates that even when the ionization cones are narrow, the shocks can be much wider angle. © 2020 The Author(s). This study was financed in part by CNPq, FAPERGS, and FAPESP. AF acknowledges the support from grant PRIN MIUR2017-20173ML3WW−001. EPM acknowledges financial support from the project ‘Estallidos6’ AYA2016-79724-C4. Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the NationalScience Foundation (United States), National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), Ministério da Ciência, Tecnologia e Inovação (Brazil), and Korea Astronomy and Space Science Institute (Republic of Korea). With funding from the Spanish government through the Severo Ochoa Centre of Excellence accreditation SEV-2017-0709. |
| Databáze: | OpenAIRE |
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