A dataset provided by the European Space Agency

Name OT1_shaileyd_1
Title Testing the XDR-High-J CO Paradigm in Nearby Galaxies
URL

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DOI 10.5270/esa-awbxyud
Author hailey-dunsheath, s.
Description One of the most exciting first results from SPIRE and PACS spectroscopy is the detection of high-J CO emission in galaxies. Such emission has long been proposed as a tracer of X-ray dominated regions (XDRs) produced by AGN, and as a powerful diagnostic tool for future millimeter-wave study of AGN at high redshift. The shortest wavelength submillimeter CO lines detected by SPIRE-FTS in the X-ray luminous ULIRG Mrk 231 are interpreted as arising from an extended XDR, providing strong observational support for the XDR-high-J CO connection. However, our group (SHINING; PI E. Sturm) has used PACS to detect even higher-J far-IR CO emission in a few nearby galaxies, including 2 starburst galaxies with little evidence of a luminous AGN. Can high-J CO emission also be produced in gas heated by the UV radiation or mechanical output of a starburst? To address this question we propose to measure a set of far-IR CO lines in 4 nearby AGN and 4 starburst galaxies, as well as in 2 merging systems with large masses of shock-heated molecular gas. Does the high-J CO line SED reflect the different excitation mechanisms in these template objects? We additionally propose to use OH line observations to estimate the abundance of this molecule, which is a sensitive tracer of X-ray-driven chemistry. The OH line profiles will also be used to search for evidence of molecular outflows, which may drive shock heating. Each of these galaxies will have SHINING GT observations of the set of far-IR fine-structure lines, which includes important tracers of UV-, X-ray-, and shock-heated gas. The AGN subsample is restricted to the most nearby systems, where the high spatial resolution of PACS is sufficient to separate the nuclear AGN-heated gas from the circumnuclear star-forming regions. The PACS CO data obtained here will provide the first well-sampled far-IR extragalactic CO line SEDs, and will be an essential reference for future high redshift studies.
Publication High-J CO Sleds in Nearby Infrared Bright Galaxies Observed By Herschel-PACS . Mashian N. et al. . The Astrophysical Journal, Volume 802, Issue 2, article id. 81, 17 pp. (2015). . 802 . 10.1088\/0004-637X\/802\/2\/81 . 2015ApJ...802...81M ,
A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns . Lu Nanyao et al. . The Astrophysical Journal Supplement Series, Volume 230, Issue 1, article id. 1, 34 pp. (2017). . 230 . 10.3847\/1538-4365\/aa6476 . 2017ApJS..230....1L ,
Instrument SPIRE_SpireSpectrometer_, PACS_PacsRangeSpec_point
Temporal Coverage 2011-08-02T09:14:25Z/2012-09-25T16:59:16Z
Version SPG v14.2.2
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-03-25T14:17:48Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-03-25T14:17:48Z, OT1_shaileyd_1, SPG v14.2.2. https://doi.org/10.5270/esa-awbxyud