2017A&A...607A.116E


C.D.S. - SIMBAD4 rel 1.7 - 2019.12.06CET15:07:20

2017A&A...607A.116E - Astronomy and Astrophysics, volume 607A, 116-116 (2017/11-1)

Outflows of hot molecular gas in ultra-luminous infrared galaxies mapped with VLT-SINFONI.

EMONTS B.H.C., COLINA L., PIQUERAS-LOPEZ J., GARCIA-BURILLO S., PEREIRA-SANTAELLA M., ARRIBAS S., LABIANO A. and ALONSO-HERRERO A.

Abstract (from CDS):

We present the detection and morphological characterization of hot molecular gas outflows in nearby ultra-luminous infrared galaxies (ULIRGs), using the Spectrograph for Integral Field Observations in the Near Infrared (SINFONI) on the Very Large Telescope (VLT). We detect outflows observed in the 2.12µm H2 1-0 S(1) line for three out of four ULIRGs that we analyzed, namely IRAS 12112+0305, IRAS 14348-1447, and IRAS 22491-1808. The outflows are mapped on scales of 0.7-1.6kpc, show typical outflow velocities of 300-500km/s, and appear to originate from the nuclear region. The outflows comprise hot molecular gas masses of MH2_ (hot)∼6–8x103^M. Assuming a hot-to-cold molecular gas mass ratio of 6x10–5, as found in nearby luminous infrared galaxies, the total (hot + cold) molecular gas mass in these outflows is expected to be MH2(tot)∼1x108M. This translates into molecular mass outflow rates of MH2(tot)∼30-85M/yr, which is a factor of a few lower than the star formation rate in these ULIRGs. In addition, most of the outflowing molecular gas does not reach the escape velocity of these merger systems, which implies that the bulk of the outflowing molecular gas is re-distributed within the system and thus remains available for future star formation. The fastest H2 outflow is seen in the Compton-thick AGN of IRAS 14348-1447, reaching a maximum outflow velocity of ∼900km/s. Another ULIRG, IRAS 17208-0014, shows asymmetric H2 line profiles different from the outflows seen in the other three ULIRGs. We discuss several alternative explanations for the line asymmetries in this system, including a very gentle galactic wind, internal gas dynamics, low-velocity gas outside the disk, or two superposed gas disks. We do not detect the hot molecular counterpart to the outflow previously detected in CO(2-1) in IRAS 17208-0014, but we note that our SINFONI data are not sensitive enough to detect this outflow if it has a small hot-to-cold molecular gas mass ratio of ≤9x10–6.

Abstract Copyright: © ESO, 2017

Journal keyword(s): galaxies: interactions - galaxies: individual: IRAS 12112+0305 - galaxies: individual: IRAS 14348-1447 - galaxies: individual: IRAS 17208-0014 - galaxies: individual: IRAS 22491-1808 - ISM: jets and outflows - ISM: jets and outflows

Simbad objects: 7

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Number of rows : 7

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NGC 3256 IG 10 27 51.284 -43 54 13.55   11.83 11.33 10.62 11.9 ~ 735 2
2 ESO 320-30 H2G 11 53 11.722 -39 07 48.72   13.30   11.86   ~ 146 1
3 LEDA 39024 LIN 12 13 46.107 +02 48 41.50           ~ 309 1
4 Mrk 231 Sy1 12 56 14.2340989340 +56 52 25.238555193   14.68 13.84     ~ 1742 3
5 2MASX J14373831-1500239 Sy1 14 37 38.317 -15 00 23.97   16.58 16.40     ~ 243 1
6 6dFGS gJ172322.0-001701 LIN 17 23 21.943 -00 17 00.96   15.1       ~ 368 0
7 NAME South America H2G 22 51 49.307 -17 52 23.96   16.97       ~ 282 3

    Equat.    Gal    SGal    Ecl

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2019.12.06-15:07:20

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