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A CO molecular gas ...
A CO molecular gas wind 340 pc away from the Seyfert 2 nucleus in ESO420-G13 probes an elusive radio jet*
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- Fernandez-Ontiveros, J. A. (författare)
- National Observatory of Athens,Universidad de la Laguna,University of La Laguna,Instituto de Astrofísica de Canarias,Istituto nazionale di astrofisica (INAF)
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- Dasyra, K. M. (författare)
- National Observatory of Athens,University of Athens
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- Hatziminaoglou, E. (författare)
- European Southern Observatory Santiago
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- Malkan, M. A. (författare)
- University of California at Los Angeles (UCLA)
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- Pereira-Santaella, M. (författare)
- Agencia Estatal Consejo Superior de Investigaciones Científicas,Spanish National Research Council,University Of Oxford
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- Papachristou, M. (författare)
- National Observatory of Athens,University of Athens
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- Spinoglio, L. (författare)
- Istituto nazionale di astrofisica (INAF)
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- Combes, F. (författare)
- Sorbonne Université,Sorbonne University
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- Aalto, Susanne, 1964 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
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- Nagar, N. (författare)
- Universidad de Concepción,University of Concepcion
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- Imanishi, M. (författare)
- The Graduate University for Advanced Studies (SOKENDAI),National Institutes of Natural Sciences (NINS)
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- Andreani, P. (författare)
- European Southern Observatory Santiago
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- Ricci, C. (författare)
- Beijing University of Technology,Universidad Diego Portales,Diego Portales University
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- Slater, R. (författare)
- Universidad Andrés Bello
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(creator_code:org_t)
- 2020-01-21
- 2020
- Engelska.
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 633
- Relaterad länk:
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https://www.aanda.or...
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https://research.cha...
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https://doi.org/10.1...
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https://research.cha...
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Abstract
Ämnesord
Stäng
- A prominent jet-driven outflow of CO(2-1) molecular gas is found along the kinematic minor axis of the Seyfert 2 galaxy ESO 420-G13, at a distance of 340-600 pc from the nucleus. The wind morphology resembles the characteristic funnel shape, formed by a highly collimated filamentary emission at the base, and likely traces the jet propagation through a tenuous medium, until a bifurcation point at 440 pc. Here the jet hits a dense molecular core and shatters, dispersing the molecular gas into several clumps and filaments within the expansion cone. We also trace the jet in ionised gas within the inner less than or similar to 340 pc using the [NeII](12.8 mu m) line emission, where the molecular gas follows a circular rotation pattern. The wind outflow carries a mass of similar to 8 x 10(6) M-circle dot at an average wind projected speed of similar to 160 km s(-1), which implies a mass outflow rate of similar to 14 M-circle dot yr(-1). Based on the structure of the outflow and the budget of energy and momentum, we discard radiation pressure from the active nucleus, star formation, and supernovae as possible launching mechanisms. ESO 420-G13 is the second case after NGC 1377 where a previously unknown jet is revealed through its interaction with the interstellar medium, suggesting that unknown jets in feeble radio nuclei might be more common than expected. Two possible jet-cloud configurations are discussed to explain an outflow at this distance from the AGN. The outflowing gas will likely not escape, thus a delay in the star formation rather than quenching is expected from this interaction, while the feedback effect would be confined within the central few hundred parsecs of the galaxy.
Ämnesord
- TEKNIK OCH TEKNOLOGIER -- Maskinteknik -- Rymd- och flygteknik (hsv//swe)
- ENGINEERING AND TECHNOLOGY -- Mechanical Engineering -- Aerospace Engineering (hsv//eng)
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
- TEKNIK OCH TEKNOLOGIER -- Maskinteknik -- Strömningsmekanik och akustik (hsv//swe)
- ENGINEERING AND TECHNOLOGY -- Mechanical Engineering -- Fluid Mechanics and Acoustics (hsv//eng)
Nyckelord
- galaxies: evolution
- submillimeter: ISM
- galaxies: individual: ESO 420-G13
- ISM: jets and outflows
- techniques: high angular resolution
- galaxies: active
Publikations- och innehållstyp
- art (ämneskategori)
- ref (ämneskategori)
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- Av författaren/redakt...
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Fernandez-Ontive ...
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Dasyra, K. M.
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Hatziminaoglou, ...
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Malkan, M. A.
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Pereira-Santaell ...
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Papachristou, M.
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visa fler...
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Spinoglio, L.
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Combes, F.
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Aalto, Susanne, ...
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Nagar, N.
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Imanishi, M.
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Andreani, P.
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Ricci, C.
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Slater, R.
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visa färre...
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