A dataset provided by the European Space Agency

Name OT2_egonza01_3
Title Excited H2O and OH as tracers of buried activity in the nuclear regions of (Ultra) Luminous Infrared Galaxies
URL

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DOI https://doi.org/10.5270/esa-60e6k3l
Author European Space Agency
Description H2O and OH are key tracers of the structure, kinematics, and activity
in the nuclear regions of (Ultra) Luminous Infrared Galaxies (ULIRGs):
with their excitation dominated by pumping by far-infrared continuum
radiation, they probe the nuclear source of the far-IR radiation and its
associated structures (disks, torus); their P-Cygni, absorption, and
emission profiles trace massive molecular outflows and possibly inflows, and
the astrophysically important associated energetics involved in the (negative)
feedback from star formation and/or AGN on the molecular gas; they probe the
physical and radiative environments (X-rays, cosmic rays, hot cores) where
they reside. In order to distinguish among the above scenarios,
we propose PACS spectroscopy of key transitions of H2O and OH in a sample of 9
bright (U)LIRGs where submillimeter H2O lines have been detected with SPIRE,
as well as key diagnostic lines of NH3 and OH+ to ascertain the formation
mechanism and implied physical processes. The proposed observations will serve
as a crucial benchmark for future routine observations of H2O with ALMA in the
distant Universe.
Publication Hidden or missing outflows in highly obscured galaxy nuclei? . Falstad N. et al. . Astronomy & Astrophysics, Volume 623, id.A29, 10 pp. . 623 . 10.1051\/0004-6361\/201834586 . 2019A&A...623A..29F ,
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 ,
Importance of radiative pumping for the excitation of the H2O submillimeter lines in galaxies . González-Alfonso Eduardo et al. . Astronomy and Astrophysics . null . null . 2022A&A...666L...3G ,
High-lying OH Absorption, [C II] Deficits, and Extreme L FIR/M H2 Ratios in Galaxies . González-Alfonso E. et al. . The Astrophysical Journal, Volume 800, Issue 1, article id. 69, 10 pp. (2015). . 800 . 10.1088\/0004-637X\/800\/1\/69 . 2015ApJ...800...69G ,
Instrument PACS_PacsRangeSpec_point
Temporal Coverage 2011-12-27T13:18:36Z/2012-12-16T12:24:33Z
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 2013-06-16T12:10:04Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Excited H2O And Oh As Tracers Of Buried Activity In The Nuclear Regions Of Openparultraclosepar Luminous Infrared Galaxies, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-60e6k3l