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molecules:ism:menco [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:menco [2020/07/06 10:13] (current) – mueller | ||
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D. T. Halfen, V. V. Ilyushin, and L. M. Ziurys,\\ | D. T. Halfen, V. V. Ilyushin, and L. M. Ziurys,\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
Several clear, slightly, and heavily blended features were detected in emission in a molecular line survey of Sagittarius B2(N) in the 4 and 3 mm wavelength region using the 12 m ARO dish. The molecule occurs in both main hot cores with similar column densities at rotational temperatures of about 25 K. It is less abundant than HNCO by about factors of 35 and 53. | Several clear, slightly, and heavily blended features were detected in emission in a molecular line survey of Sagittarius B2(N) in the 4 and 3 mm wavelength region using the 12 m ARO dish. The molecule occurs in both main hot cores with similar column densities at rotational temperatures of about 25 K. It is less abundant than HNCO by about factors of 35 and 53. | ||
- | J. Cernicharo1, Z. Kisiel, B. Tercero, L. Kolesniková, | + | J. Cernicharo, Z. Kisiel, B. Tercero, L. Kolesniková, |
reported on the\\ | reported on the\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
Using extensive Orion KL molecular line survey data obtained with the IRAM 30 m telescope as well as ALMA Cycle 0 science verification data, the authors identified a plethora of transitions and characterized the physcal conditions.\\ | Using extensive Orion KL molecular line survey data obtained with the IRAM 30 m telescope as well as ALMA Cycle 0 science verification data, the authors identified a plethora of transitions and characterized the physcal conditions.\\ | ||
Using the meanwhile public IRAM 30 m data on Sagittarius B2 from\\ | Using the meanwhile public IRAM 30 m data on Sagittarius B2 from\\ | ||
A. Belloche, H. S. P. Müller, K. M. Menten, P. Schilke, and C. Comito:\\ | A. Belloche, H. S. P. Müller, K. M. Menten, P. Schilke, and C. Comito:\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
the authors also corrected and added assignments from the first paper and reanalyzed the physical conditions in that source. They find methynol, HNCO, and methyl cyanide to be more abundant in Sgr B2(N) by factors of about 40, 40, and 50, different from the two positions in Orion KL: 400, 15, and 10 for position A, and 200, 15, and 25 for position B. | the authors also corrected and added assignments from the first paper and reanalyzed the physical conditions in that source. They find methynol, HNCO, and methyl cyanide to be more abundant in Sgr B2(N) by factors of about 40, 40, and 50, different from the two positions in Orion KL: 400, 15, and 10 for position A, and 200, 15, and 25 for position B. |