| 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 byIRAS. Nicknamed the fire and ice galaxy since its widely-cited firstSpitzer-IRS observations were published in 2004, this galaxy hascontinued to amaze. Not only does it host the possibly most deeplyobscured powerful AGN/quasar in the Local Universe (z<0.4), itsextremely wide mid-IR neon line profiles and the extended red wing tothe CO(J=1-0) line hint at massive outflows. These outflows may bepowered by the radio jets, which appear to be young and which may beresponsible for the optically-obscured, highly disturbed ionized neongas line emission seen with Spitzer, the multiple spatial andkinematic O III 5007A components, and the off-nuclear soft X-raybubble seen by XMM.So far this luminous z=0.328 merger has remained unobserved byHerschel. Here we propose to study its nuclear outflow at far-infraredwavelengths to reveal optically obscured high-velocity ionized gasoutflow components, and to assess the extent and timescale of theneutral and molecular gas outflows, which may drive the evolution ofIRAS F00183-7111 from a deeply buried merger remnant to a nakedQSO. Our proposed observations may also benefit existing HerschelULIRG outflow studies by providing measurements for a ULIRG that willextend the current L(AGN) range by a factor of two. This study willfurther also be r^ant for understanding the population of deeplyobscured radio galaxies found at high redshifts. |
| Publication |
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| 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 |
| Last Update | 2025-01-24 |
| Keywords | Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, spoon et al., 2013, 'Probing the multi-phase outflows in the Fire and Ice' galaxy IRAS F00183-7111 using far-IR PACS spectroscopy', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-m2u4v2a |