| Name | OT2_hspoon_1 |
| Title | Probing the multi-phase outflows in the 'Fire and Ice. galaxy IRAS F00183-7111 using far-IR PACS spectroscopy |
| URL | http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245249&instrument_name=PACS&product_level=LEVEL0&compress=true |
| DOI | https://doi.org/10.5270/esa-m2u4v2a |
| Author | spoon, h. |
| Description | IRAS F00183-7111 is possibly the most luminous ULIRG discovered by IRAS. Nicknamed the .fire and ice galaxy. since its widely-cited first Spitzer-IRS observations were published in 2004, this galaxy has continued to amaze. Not only does it host the possibly most deeply obscured powerful AGN-quasar in the Local Universe (z<0.4), its extremely wide mid-IR neon line profiles and the extended red wing to the CO(J=1-0) line hint at massive outflows. These outflows may be powered by the radio jets, which appear to be young and which may be responsible for the optically-obscured, highly disturbed ionized neon gas line emission seen with Spitzer, the multiple spatial and kinematic [O III] 5007A components, and the off-nuclear soft X-ray bubble seen by XMM. So far this luminous z=0.328 merger has remained unobserved by Herschel. Here we propose to study its nuclear outflow at far-infrared wavelengths to reveal optically obscured high-velocity ionized gas outflow components, and to assess the extent and timescale of the neutral and molecular gas outflows, which may drive the evolution of IRAS F00183-7111 from a deeply buried merger remnant to a naked QSO. Our proposed observations may also benefit existing Herschel ULIRG outflow studies by providing measurements for a ULIRG that will extend the current L(AGN) range by a factor of two. This study will further also be r^ant for understanding the population of deeply obscured radio galaxies found at high redshifts. |
| Publication | Far-infrared Line Spectra of Active Galaxies from the Herschel-PACS Spectrometer: The Complete Database . Fernández-Ontiveros Juan Antonio et al. . The Astrophysical Journal Supplement Series, Volume 226, Issue 2, article id. 19, 26 pp. (2016). . 226 . 10.3847/0067-0049/226/2/19 . 2016ApJS..226...19F , Herschel-PACS OH Spectroscopy of Seyfert, LINER, and Starburst Galaxies . Runco Jordan N. et al. . The Astrophysical Journal . null . null . 2020ApJ...905...57R , |
| Instrument | PACS_PacsRangeSpec_point |
| Temporal Coverage | 2012-05-02T12:47:53Z/2013-01-07T10:58:08Z |
| Version | SPG v14.2.0 |
| Mission Description | Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities. |
| Creator Contact | https://support.cosmos.esa.int/h®erschel/ |
| Date Published | 2013-07-07T08:31:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2013-07-07T08:31:00Z, OT2_hspoon_1, SPG v14.2.0. https://doi.org/10.5270/esa-m2u4v2a |