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

Journal article (2005)

Authors

A. Castets Observatoire Aquitain des Sciences de l'Univers
E. Caux Centre d'Etude Spatiale des Rayonnements
A. G.G.M. Tielens Rijksuniversiteit Groningen
E. Van Dischoeck Universiteit Leiden
V. Wakelam Observatoire Aquitain des Sciences de l'Univers
A Walters Centre d'Etude Spatiale des Rayonnements
A. Bacmann Observatoire Aquitain des Sciences de l'Univers
S.M. 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
Affiliation
External organisation
ISM: molecules ISM: abundances Stars: Formation
More Info
expand_more

Published Date

2005

Language

English

Reuse Rights

Other than for strictly personal use, it is not permitted to download, forward or distribute the text or part of it, without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license such as Creative Commons.

Affiliation

External organisation

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.