A dataset provided by the European Space Agency

Name OT2_jhewitt_2
Title Understanding Shock Oxygen Chemistry in Interacting Supernova Remnants
URL

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DOI 10.5270/esa-hnbuewi
Author hewitt, j.
Description Supernova remnants interacting with dense moelcular clouds provide astrochemical laboratories to study heating and cooling of the dense ISM, shock chemistry, destruction and sputtering of dust, and the reformation of molecules. Water is expected to be a major coolant for shocks into dense gas, yet the number of remnants in which IR lines of hydroxyl and water are detected is very limited. We propose Herschel PACS, SPIRE and HIFI observations of three remnants with particularly high shocked gas densities, high dust and IR line luinosities, and extreme ionization environments. The scientific objectives of this proposal are: (1) to determine the abundance and excitation of oxygen-bearing molecules, and (2) to study the effects of variable ionization sources on oxygen chemistry in dense molecular gas shocked by powerful supernova remnant blast waves.
Publication
Instrument SPIRE_SpireSpectrometer_, HIFI_HifiPoint_pos, PACS_PacsLineSpec_point
Temporal Coverage 2012-09-20T09:04:20Z/2012-10-08T15:58:36Z
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 2013-04-08T15:00:18Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-04-08T15:00:18Z, OT2_jhewitt_2, SPG v14.2.0. https://doi.org/10.5270/esa-hnbuewi