An unbiased (sub)millimeter spectral survey of the solar-type protostar IRAS 16293-2422

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An unbiased (sub)millimeter spectral survey of the solar-type protostar IRAS 16293-2422

Journal Article (2005)

Author(s)

A. Castets (Observatoire Aquitain des Sciences de l'Univers)

E. Caux (Centre d'Etude Spatiale des Rayonnements)

A. Bacmann (Observatoire Aquitain des Sciences de l'Univers)

S. Cazaux (INAF-Osservatorio Astrofisico di Arcetri)

C. Ceccarelli (Laboratoire d'Astrophysique de Grenoble)

C. Comito (Max-Planck-Institute for Radio Astronomy)

F Helmich (SRON–Netherlands Institute for Space Research)

C. Kahane (Laboratoire d'Astrophysique de Grenoble)

B. Parise (Centre d'Etude Spatiale des Rayonnements)

P. Shilke (Max-Planck-Institute for Radio Astronomy)

A. G.G.M. Tielens (Rijksuniversiteit Groningen)

E. Van Dischoeck (Universiteit Leiden)

Valentine Wakelam (Observatoire Aquitain des Sciences de l'Univers)

A Walters (Centre d'Etude Spatiale des Rayonnements)

Affiliation

External organisation

ISM: molecules ISM: abundances Stars: Formation

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Publication Year

2005

Language

English

Affiliation

External organisation

Issue number

577

Pages (from-to)

345-346

Downloads counter

215

Abstract

We present the first results of a systematic (sub)millimeter unbiased spectral line survey performed with the IRAM-30m and JCMT radiotele-scopes towards the low-mass protostar IRAS 16293-2422 (IRAS16293). When completed this survey will cover most of the frequency band attainable with the 30m (80-280 GHz) and with the JCMT in the 350 GHz band (335-365 GHz), i.e. 201 GHz.

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