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molecules:ism:menh2 [2022/04/27 16:38] – mueller | molecules:ism:menh2 [2023/09/05 14:43] (current) – mueller | ||
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**[[https:// | **[[https:// | ||
// | // | ||
- | They used the Mitaka 6 m telescope for the //a//, 5< | + | They used the Mitaka 6 m telescope for the //a//-symmetry |
\\ | \\ | ||
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At the same time,\\ | At the same time,\\ | ||
N. Fourikis, K. Takagi, and M. Morimoto\\ | N. Fourikis, K. Takagi, and M. Morimoto\\ | ||
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They used the Parkes 64 m telecope to detect the transition near 8.8 GHz in emission toward Sagittarius B2.\\ | They used the Parkes 64 m telecope to detect the transition near 8.8 GHz in emission toward Sagittarius B2.\\ | ||
\\ | \\ | ||
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Both papers mentioned above reported also the detection toward the Orion A molecular cloud, however, these detections are incorrect, see e.g.\\ | Both papers mentioned above reported also the detection toward the Orion A molecular cloud, however, these detections are incorrect, see e.g.\\ | ||
L. E. B. Johansson, C. Andersson, J. Elldér, P. Friberg, Å. Hjalmarson, B. Höglund, W. M. Irvine, H. Olofsson, and G. Rydbeck,\\ | L. E. B. Johansson, C. Andersson, J. Elldér, P. Friberg, Å. Hjalmarson, B. Höglund, W. M. Irvine, H. Olofsson, and G. Rydbeck,\\ | ||
**[[https:// | **[[https:// | ||
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
- | \\ | + | \\ |
+ | |||
+ | T. Kamiński, K. M. Menten, R. Tylenda, A. Karakas, A. Belloche, and N. A. Patel\\ | ||
+ | investigated the\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | Methylamine was identified through several transitions covered by the IRAM 30 m and APEX 12 m telescopes.\\ | ||
+ | \\ | ||
S. Zeng, I. Jiménez-Serra, | S. Zeng, I. Jiménez-Serra, | ||
carried out a study on\\ | carried out a study on\\ | ||
**[[https:// | **[[https:// | ||
+ | //Mon. Not. R. Astron. Soc.// **478**, 2962–2975 (2018).\\ | ||
They performed an unbiased molecular line survey of the quiescent molecular cloud G+0.693−0.03 using the GBT 100 m dish (12.7–15.5 GHz and sections of 18–27 GHz) and the IRAM 30 m dish (80–116, 128–176, and 240–272 GHz). The detected five lines of methylamine.\\ | They performed an unbiased molecular line survey of the quiescent molecular cloud G+0.693−0.03 using the GBT 100 m dish (12.7–15.5 GHz and sections of 18–27 GHz) and the IRAM 30 m dish (80–116, 128–176, and 240–272 GHz). The detected five lines of methylamine.\\ | ||
- | \\ | + | \\ |
E. G. Bøgelund, B. A. McGuire, M. R. Hogerheijde, | E. G. Bøgelund, B. A. McGuire, M. R. Hogerheijde, | ||
reported on\\ | reported on\\ | ||
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//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The authors describe the first unambigous detection of methylamine outside of the Galactic center.\\ | The authors describe the first unambigous detection of methylamine outside of the Galactic center.\\ | ||
+ | \\ | ||
+ | P. Gyawali, R. A. Motiyenko, A. Belloche, I. Kleiner, V. V. Ilyushin, E. A. Alekseev, I. Gulaczyk and M. Kreglewski\\ | ||
+ | described the\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | Five lines in // | ||
+ | \\ | ||
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- | Contributor(s): | + | Contributor(s): |
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