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

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

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..345c&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Computer Science

Ism: Molecules, Ism: Abundances, Stars: Formation

Scientific paper

We present the first results of a systematic (sub)millimeter unbiased spectral line survey performed with the IRAM-30m and JCMT radiotelescopes 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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