A dataset provided by the European Space Agency

Name OT1_rmeijeri_1
Title Gas excitation through black hole accretion and star formation in the centers of active galaxies.
URL

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DOI 10.5270/esa-mitjanj
Author meijerink, r.
Description Stunning observations with SPIRE FTS of Mrk 231 have shown that CO lines are very bright up to J=13-12, and there is no sign of a decline in the CO Spectral Line Energy Distribution (SLED). Our SPIRE FTS spectra show that this is a common feature of AGN type galaxies. Therefore, we propose to observe a set of 4 very high-J CO line transitions using the PACS spectrometer, for 5 of these well studied proto-typical (Ultra-)Luminous Infrared Galaxies ((U)LIRGs) and one starburst galaxy. The question of the relative role and contribution of AGN to the far-infrared luminosities of local (U)LIRG systems has long been a problem in our understanding of the evolutionary path of these objects, and as well for the interpretation of deep far-infrared surveys. Our SPIRE FTS and our ground-based CO line observations together with the PACS observations in this program will allow us, for the first time, to complete a full CO SLED for a set of (U)LIRGs. Combining this with our models of Photon Dominated Regions (PDRs) and X-ray Dominated Regions (XDRs), we will then be able to determine the physical state of the interstellar medium and estimate the starburst-AGN contribution to the total energetics of these systems.
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 ,
Instrument PACS_PacsRangeSpec_point
Temporal Coverage 2010-12-31T13:10:10Z/2012-08-24T07:39:09Z
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 2013-02-24T07:03:21Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-02-24T07:03:21Z, OT1_rmeijeri_1, SPG v14.2.0. https://doi.org/10.5270/esa-mitjanj