A dataset provided by the European Space Agency

Name OT1_pogle01_1
Title Radio Jet Feedback on Molecular and Atomic Gas in Radio Galaxies
URL

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DOI 10.5270/esa-1mh8zzw
Author ogle, p.
Description We propose Herschel SPIRE and PACS atomic and molecular line spectroscopy and photometry of 23 H2-luminous radio galaxies. Most of these galaxies are IR-weak, such that the kinetic energy output of the radio jet dominates over the radiative output from the AGN accretion disk and star formation in the host galaxy. This new class of galaxies, discovered by Spitzer, has unique MIR spectra with very strong H2 rotational emission lines but weak PAH features compared to normal star-forming galaxies. We may be seeing the direct effects of AGN radio jet feedback, dramatically and fundamentally disturbing the host galaxy interstellar medium in a way that suppresses star formation. Herschel spectroscopy and photometry are essential to inventory the mass and energetics of the atomic and molecular ISM over a wide range of densities and temperatures, and thereby obtain a better understanding of the radio jet feedback mechanism that regulates massive galaxy evolution. We will use shock models to interpret the [O I] and CO emission line spectra and determine the density, temperature, and energetics of shocked molecular gas. Herschel photometry will probe the peak of the IR SED and yield estimates of the total mass of cold dust and cold molecular gas. This will allow us to assess what fraction of the molecular ISM is disturbed by shocks, and understand why and to what extent star formation is suppressed by radio jet feedback.
Publication Star Formation Suppression Due to Jet Feedback in Radio Galaxies with Shocked Warm Molecular Gas . Lanz Lauranne et al. . The Astrophysical Journal, Volume 826, Issue 1, article id. 29, 40 pp. (2016). . 826 . 10.3847\/0004-637X\/826\/1\/29 . 2016ApJ...826...29L ,
Instrument SPIRE_SpireSpectrometer_, PACS_PacsPhoto_largeScan, PACS_PacsRangeSpec_point, SPIRE_SpirePhoto_small
Temporal Coverage 2011-07-11T19:43:35Z/2012-11-23T03:22:38Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-05-23T00:29:46Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-05-23T00:29:46Z, OT1_pogle01_1, SPG v14.2.0. https://doi.org/10.5270/esa-1mh8zzw