This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revisionLast revisionBoth sides next revision |
molecules:ism:dme [2021/08/24 13:30] – mueller | molecules:ism:dme [2021/08/24 13:37] – mueller |
---|
reported on the\\ | reported on the\\ |
**[[https://doi.org/10.1051/0004-6361/202141282|Laboratory Rotational Spectra of Doubly Deuterated Dimethyl Ether (CH<sub>3</sub>OCHD<sub>2</sub>) — First ALMA Detection in the Interstellar Medium]]**\\ | **[[https://doi.org/10.1051/0004-6361/202141282|Laboratory Rotational Spectra of Doubly Deuterated Dimethyl Ether (CH<sub>3</sub>OCHD<sub>2</sub>) — First ALMA Detection in the Interstellar Medium]]**\\ |
//Astron. Astrophys.// **651**, Art. No. A120 (2013).\\ | //Astron. Astrophys.// **651**, Art. No. A120 (2021).\\ |
The isotopolog was detected in the course of the Protostellar Interferometric Line Survey (PILS) of IRAS 16293−2422 with ALMA between | The isotopolog was detected through numerous transitions in the course of the Protostellar Interferometric Line Survey (PILS) of IRAS 16293−2422 with ALMA between 329.1 and 362.9 GHz. The column density of this doubly deuterated isotopolog is roughly a factor of five higher than what would be extrapolated from the un- and sinly deuterated isotopologs, as frequently observed in this as well as other sources.\\ |
| |
| |