1. DISCOVERY OF AN ACTIVE GALACTIC NUCLEUS DRIVEN MOLECULAR OUTFLOW IN THE LOCAL EARLY-TYPE GALAXY NGC 1266
- Author
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Timothy A. Davis, Anne-Marie Weijmans, Leo Blitz, Sadegh Khochfar, K. Shapiro, Frédéric Bournaud, Nicholas Scott, Lisa M. Young, Davor Krajnović, Richard M. McDermid, Katherine Alatalo, Pierre Yves Lablanche, Jesus Falcon-Barosso, Laura A. Lopez, Maxime Bois, Pierre-Alain Duc, Eric Emsellem, Roger L. Davies, Paolo Serra, Harald Kuntschner, Tom Oosterloo, Raffaella Morganti, Thorsten Naab, Alison F. Crocker, Martin Bureau, Marc Sarzi, Sergio Martín, P. T. de Zeeuw, Michele Cappellari, Department of Astronomy, University of California, Physics Department, New Mexico Tech, Socorro, Sub-department of Astrophysics, Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Department of Astronomy and Astrophysics, University of California, Aerospace Research Laboratories, Northrop Grumman Aerospace Systems, Department of Astronomy, University of Massachusetts, European Southern Observatory, Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), European Southern Observatory (ESO), Instituto de Astrofísica de Canarias (IAC), Max-Planck-Institut für Extraterrestriche Physik (MPE), Gemini Observatory, Netherlands Institute for Radio Astronomy (ASTRON), Max-Planck-Institut für Astrophysik (MPA), University of Hertfordshire [Hatfield] (UH), Dunlap Institute for Astronomy and Astrophysics, University of Toronto, and Astronomy
- Subjects
Angular momentum ,Active galactic nucleus ,Milky Way ,Astrophysics::High Energy Astrophysical Phenomena ,RADIO GALAXIES ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,ELLIPTIC GALAXIES ,0103 physical sciences ,STAR-FORMING GALAXIES ,Astrophysics::Solar and Stellar Astrophysics ,NEARBY GALAXIES ,IC 5063 ,BLACK-HOLES ,010303 astronomy & astrophysics ,galaxies: kinematics and dynamics ,Astrophysics::Galaxy Astrophysics ,Physics ,Field galaxy ,010308 nuclear & particles physics ,Star formation ,Molecular cloud ,Astronomy and Astrophysics ,SAURON PROJECT ,Galaxy ,SPITZER ,ISM: jets and outflows ,GAS ,Space and Planetary Science ,MULTI-GAUSSIAN EXPANSION ,Outflow ,Astrophysics::Earth and Planetary Astrophysics ,galaxies: evolution ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,galaxies: ISM - Abstract
International audience; We report the discovery of a powerful molecular wind from the nucleus of the non-interacting nearby S0 field galaxy NGC 1266. The single-dish CO profile exhibits emission to ±400 km s-1 and requires a nested Gaussian fit to be properly described. Interferometric observations reveal a massive, centrally concentrated molecular component with a mass of 1.1 × 109 M sun and a molecular outflow with a molecular mass of ≈2.4 × 107 M sun. The molecular gas close to the systemic velocity consists of a rotating, compact nucleus with a mass of about 4.1 × 108 M sun within a radius of ≈60 pc. This compact molecular nucleus has a surface density of ≈2.7 × 104 M sun pc-2, more than two orders of magnitude larger than that of giant molecular clouds in the disk of the Milky Way, and it appears to sit on the Kennicutt-Schmidt relation despite its extreme kinematics and energetic activity. We interpret this nucleus as a disk that confines the outflowing wind. A mass outflow rate of ≈13 M sun yr-1 leads to a depletion timescale of lsim85 Myr. The star formation in NGC 1266 is insufficient to drive the outflow, and thus it is likely driven by the active galactic nucleus. The concentration of the majority of the molecular gas in the central 100 pc requires an extraordinary loss of angular momentum, but no obvious companion or interacting galaxy is present to enable the transfer. NGC 1266 is the first known outflowing molecular system that does not show any evidence of a recent interaction.
- Published
- 2011