A dataset provided by the European Space Agency

Name OT2_mbenedet_1
Title SPECSO: Spectroscopy of Shocks in Outflows
URL

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DOI 10.5270/esa-fhqmag0
Author benedettini, m.
Description In the early protostellar stages, fast jets powered by the nascent star, possibly surrounded by a wider angle wind, are seen to interact with the parental medium through molecular bowshocks, producing a slower moving molecular outflow cavity. The nature of the shock accelerating the outflow plays an important role in the dynamical and chemical evolution of the entrained gas. We propose to study with Herschel the physics of protostellar outflow shocks from the observation of CO and OI lines with HIFI and PACS, in a broad sample of outflows. These observations will permit to bring strong constraints to shock models over a wide range of parameters, and will facilitate the interpretation of current observational programs on protostellar shock chemistry and dynamics.
Publication The shocked gas of the BHR71 outflow observed by Herschel: indirect evidence for an atomic jet . Benedettini M. et al. . Astronomy & Astrophysics, Volume 598, id.A14, 16 pp. . 598 . 10.1051\/0004-6361\/201629451 . 2017A&A...598A..14B ,
Instrument HIFI_HifiPoint_dbs, PACS_PacsLineSpec_point
Temporal Coverage 2012-08-16T14:39:34Z/2013-03-26T22:54:29Z
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 2013-09-26T22:25:34Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-09-26T22:25:34Z, OT2_mbenedet_1, SPG v14.2.0. https://doi.org/10.5270/esa-fhqmag0