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- | This report is actually the first one on an umambiguous (i.e. multi line) detection of propenal in the ISM. It is also the first one on the detection of warm (~125 K) propenal in the ISM as well as on the detection of propanal around a low-mass protostar. The Protostellar Interferometric Line Survey (PILS) was carried out with ALMA in its Band 7 (329 – 363 GHz) with additional observations in Band 6. A total of 15 different unblended (with respect to a different molecule) lines were identified. | + | This report is actually the first one on an umambiguous (i.e. multi line) detection of propenal in the ISM. It is also the first one on the detection of warm (~125 K) propenal in the ISM and on the detection of propanal around a low-mass protostar. The Protostellar Interferometric Line Survey (PILS) was carried out with ALMA in its Band 7 (329 – 363 GHz) with additional observations in Band 6. A total of 15 different unblended (with respect to a different molecule) lines were identified. |
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