This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision | |
| molecules:ism:ch3chco [2023/03/06 12:13] – mueller | molecules:ism:ch3chco [2023/03/06 12:20] (current) – mueller |
|---|
| **[[https://doi.org/10.1051/0004-6361/202245732|Discovery of CH<sub>3</sub>CHCO in TMC-1 with the QUIJOTE Line Survey]]**\\ | **[[https://doi.org/10.1051/0004-6361/202245732|Discovery of CH<sub>3</sub>CHCO in TMC-1 with the QUIJOTE Line Survey]]**\\ |
| //Astron. Astrophys.// **671**, (2023), Art. No. L6.\\ | //Astron. Astrophys.// **671**, (2023), Art. No. L6.\\ |
| Ten rotational transitions with 3 ≤ //J// ≤ 5 and //K<sub>a</sub>// were identified with resolved methyl internal rotation splitting. A sufficiently large fraction of the lines is not or only marginally blended and above the 3//σ// noise level. | Ten rotational transitions with 3 ≤ //J// ≤ 5 and //K<sub>a</sub>// were identified with resolved methyl internal rotation splitting. A sufficiently large fraction of the lines is not or only marginally blended and above the 3//σ// noise level. The ketene to methylketene ratio is ~93; the ratio of methylketene to it isomer //trans//-propenal is about 2/3.\\ |
| \\ | \\ |
| |