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.
|Number of pages||2|
|Journal||European Space Agency, (Special Publication) ESA SP|
|Publication status||Published - 2005|
- ISM: abundances Stars: Formation
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