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molecules:ism:methoxymethanol [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:methoxymethanol [2020/03/10 09:18] (current) – mueller | ||
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===== On the Detection of Methoxymethanol, | ===== On the Detection of Methoxymethanol, | ||
- | B. A. McGuire, C. N. Shingledecker, | + | B. A. McGuire, C. N. Shingledecker, |
reported on the\\ | reported on the\\ | ||
**[[https:// | **[[https:// | ||
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More than two dozen unblended or essentially unblended transitions were detected in several small recordings in Bands 6 and 7 through observations of the high-mass starforming region NGC 6334I-MM1. Assuming an excitation temperature of 200 K, its column density was found to be lower than that of methanol by a factor slightly larger than 30. | More than two dozen unblended or essentially unblended transitions were detected in several small recordings in Bands 6 and 7 through observations of the high-mass starforming region NGC 6334I-MM1. Assuming an excitation temperature of 200 K, its column density was found to be lower than that of methanol by a factor slightly larger than 30. | ||
+ | B. Tercero, S. Cuadrado, A. López, N. Brouillet, D. Despois, and J. Cernicharo\\ | ||
+ | investigated\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | They analyzed the Cycle 0 ALMA science verification data and found methoxymethanol besides several other molecules. | ||
- | ---- | + | S. Manigand, J. K. Jørgensen, H. Calcutt, H. S. P. Müller, N. F. W. Ligterink, A. Coutens, M. N. Drozdovskaya, |
+ | reported on\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | They found methoxymethanol toward the low-mass proto-star IRAS 16293–2422 B in this context. | ||
- | Contributor(s): | ||
+ | ---- | ||
+ | |||
+ | Contributor(s): | ||
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