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molecules:ism:mgc2_4h [2021/09/03 16:50] – mueller | molecules:ism:mgc2_4h [2021/09/03 16:54] – mueller |
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Eight transitions with //N'// = 9 to 16 between 89 and 169 GHz were shown. Two transitions (//N'// = 9 and 10) are clearly visible with two fine structure components. One component of the //N'// = 11 transition appears to be not or only slightly blended. The remainder of the lines are difficult to asses without modeling results because of blending or poorer signal-to-noise ratios.\\ | Eight transitions with //N'// = 9 to 16 between 89 and 169 GHz were shown. Two transitions (//N'// = 9 and 10) are clearly visible with two fine structure components. One component of the //N'// = 11 transition appears to be not or only slightly blended. The remainder of the lines are difficult to asses without modeling results because of blending or poorer signal-to-noise ratios.\\ |
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M. Agúndez, J. Cernicharo, and M. Guélin\\ | M. Agúndez, J. Cernicharo, and M. Guélin\\ |
had earlier reported on\\ | had earlier reported on\\ |
**[[https://doi.org/10.1051/0004-6361/201424542|New molecules in IRC +10216: confirmation of C<sub>5</sub>S and tentative identification of MgCCH, NCCP, and SiH<sub>3</sub>CN]]**\\ | **[[https://doi.org/10.1051/0004-6361/201424542|New molecules in IRC +10216: confirmation of C<sub>5</sub>S and tentative identification of MgCCH, NCCP, and SiH<sub>3</sub>CN]]**\\ |
//Astron. Astrophys.// **570**, Art. No. A45 (2014).\\ | //Astron. Astrophys.// **570**, Art. No. A45 (2014).\\ |
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| J. R. Pardo, C. Cabezas, J. P. Fonfría, M. Agúndez, B. Tercero, P. de Vicente, M. Guélin and J. Cernicharo |
| reported on\\ |
| **[[https://doi.org/10.1051/0004-6361/202141671|Magnesium Radicals MgC<sub>5</sub>N and MgC<sub>6</sub>H in IRC +10216]]**\\ |
| //Astron. Astrophys.// **652**, Art. No. L13 (2021).\\ |
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