The TELPERION survey for distant [O iii ] clouds around luminous and hibernating AGN
| Autor: | William C Keel, Alexei Moiseev, D V Kozlova, A I Ikhsanova, D V Oparin, R I Uklein, A A Smirnova, M V Eselevich |
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| Rok vydání: | 2021 |
| Předmět: |
ACTIVE GALACTIC NUCLEI
Astrophysics::High Energy Astrophysical Phenomena FOS: Physical sciences LINE SURVEY Astrophysics::Cosmology and Extragalactic Astrophysics INTERACTIONS [GALAXIES] NARROW BANDS INTEGRATED CIRCUITS BROAD BANDS Astrophysics::Solar and Stellar Astrophysics MERGING ACTIVE [GALAXIES] Astrophysics::Galaxy Astrophysics ELECTROMAGNETIC WAVE EMISSION GALAXIES ACTIVE SEYFERT [GALAXY] Astronomy and Astrophysics BUDGET CONTROL Astrophysics - Astrophysics of Galaxies WIDE-FIELD GALAXIES SEYFERT [GALAXIES] Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) EMISSION LINES IMAGING SURVEYS SURVEYS |
| Zdroj: | Monthly Notices of the Royal Astronomical Society |
| ISSN: | 1365-2966 0035-8711 |
| DOI: | 10.1093/mnras/stab3656 |
| Popis: | We present a narrowband [O III] imaging survey of 111 AGN hosts and 17 merging-galaxy systems, in search of distant extended emission-line regions (EELRs) around AGN (either extant or faded). Our data reach deeper than detection from the broadband SDSS data, and cover a wider field than some early emission-line surveys used to study extended structure around AGN. Spectroscopic followup confirms two new distant AGN-ionized clouds, in the merging systems NGC 235 and NGC 5514, projected at 26 and 75 kpc from the nuclei (respectively). We also recover the previously-known region in NGC 7252. These results strengthen the connection between EELRs and tidal features; kinematically quiescent distant EELRs are virtually always photoionized tidal debris. We see them in ~10% of the galaxies in our sample with tidal tails. Energy budgets suggest that the AGN in NGC 5514 has faded by >3 times during the extra light-travel time ~250,000 years from the nucleus to the cloud and then to the observer; strong shock emission in outflows masks the optical signature of the AGN. For NGC 235 our data are consistent with but do not unequivocally require variation over ~85,000 years. In addition to these very distant ionized clouds, luminous and extensive line emission within four galaxies - IC 1481, ESO 362-G08, NGC 5514, and NGC 7679. IC 1481 shows apparent ionization cones, a rare combination with its LINER AGN spectrum. In NGC 5514, we measure a 7-kpc shell expanding at ~370 km/s west of the nucleus. Accepted for MNRAS |
| Databáze: | OpenAIRE |
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