A dataset provided by the European Space Agency

Name OT2_lolmi_3
Title The physical and chemical state of high-mass pre- and proto-stellar cores identified by the Hi-GAL survey
URL

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DOI 10.5270/esa-b239q6q
Author olmi, l.
Description We propose to investigate the physical, chemical and dynamical properties of a sample of newly found high-mass pre- and proto-stellar cores identified by the ''Herschel infrared GALactic Plane Survey.. (Hi-GAL; Molinari et al. 2010). We will perform observations of the o-NH3(1_0-0_0) line (and, simultaneously, also of the o-H2O(1_10-1_01) transition) that will allow us to identify both similarities and differences between the physical and chemical conditions before and after the formation of a warm-hot source inside the dusty core identified in the SPIRE-PACS maps. Hence, these observations will improve our knowledge of the earliest phases in the evolution of high-mass stars. We will also attempt the detection of the NH(1-0) line towards a smaller sample of sources, in order to improve our knowledge of the N-chemistry during early high-mass star formation.
Publication Herschel-HIFI observations of H2O, NH3, and N2H+ toward high-mass starless and protostellar clumps identified by the Hi-GAL survey⋆ . Olmi L. et al. . Astronomy & Astrophysics, Volume 583, id.A125, 28 pp. . 583 . 10.1051\/0004-6361\/201526901 . 2015A&A...583A.125O ,
Instrument HIFI_HifiPoint_pos
Temporal Coverage 2013-04-19T17:58:25Z/2013-04-20T07:42:40Z
Version SPG v14.1.0
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/herschel/
Date Published 2013-10-20T07:38:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-20T07:38:00Z, OT2_lolmi_3, SPG v14.1.0. https://doi.org/10.5270/esa-b239q6q