MOTTRAM, J. C.,; KRISTENSEN, L. E.,; VAN DISHOECK, E. F.,; BRUDERER, S.,; SAN JOSE-GARCIA, I.,; KARSKA, A.,; VISSER, R.,; SANTANGELO, G.,; BENZ, A. O.,; BERGIN, E. A.,; CASELLI, P.,; HERPIN, Fabrice; HOGERHEIJDE, M. R.,; JOHNSTONE, D.,; VAN KEMPEN, T. A.,; LISEAU, R.,; NISINI, B.,; TAFALLA, M.,; VAN DER TAK, F. F. S.,; WYROWSKI, F.,

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MOTTRAM, J. C.,

KRISTENSEN, L. E.,
Leiden Observatory [Leiden]

VAN DISHOECK, E. F.,
Max-Planck-Institut für Extraterrestrische Physik [MPE]
Leiden Observatory [Leiden]

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2014-11p. 29021

Résumé en anglais

This sample was the target of a series of observations of gas-phase water transitions with the Heterodyne Instrument for the Far-Infrared (HIFI) on Herschel between March 2010 and October 2011. Three of the Class I sources (IRAS3A, RCrA-IRS5A and HH100-IRS) were only observed in the 557GHz H2O 110-101 line, which was presented for all sources by Kristensen et al. (2012A&A...542A...8K). All other sources were observed in between four and seven H216O transitions and between one and four H218O transitions. Additional data from two OT2 programmes, OT2rvisser2 and OT2evandish4, are also included to augment the WISH data.(2 data files).< Réduire

Mots clés en anglais

YSOs

Spectroscopy

Origine

Importé de hal

Unités de recherche

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804