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| molecules:ism:hcco [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:hcco [2019/10/22 17:10] (current) – mueller |
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| M. Agúndez, J. Cernicharo, and M. Guélin\\ | M. Agúndez, J. Cernicharo, and M. Guélin\\ |
| reported on the\\ | reported on the\\ |
| **[[http://dx.doi.org/10.1051/0004-6361/201526317|Discovery of Interstellar Ketenyl (HCCO), a Surprisingly Abundant Radical]]**\\ | **[[https://doi.org/10.1051/0004-6361/201526317|Discovery of Interstellar Ketenyl (HCCO), a Surprisingly Abundant Radical]]**\\ |
| //Astron. Astrophys.// **577**, Art. No. L5 (2015).\\ | //Astron. Astrophys.// **577**, Art. No. L5 (2015).\\ |
| The IRAM 30 m telescope was used to detect the four Δ//F// = Δ//J// = Δ//N// hyperfine components with //N// = 4 – 3 near 86.65 GHz toward the dense core Lupus-1A, which is in the vicinity of the low-mass protostar IRAS 15398-3359, and toward the the young stellar object IRAS 18148–0440 in the L483 dense core. | The IRAM 30 m telescope was used to detect the four Δ//F// = Δ//J// = Δ//N// hyperfine components with //N// = 4 – 3 near 86.65 GHz toward the dense core Lupus-1A, which is in the vicinity of the low-mass protostar IRAS 15398-3359, and toward the the young stellar object IRAS 18148–0440 in the L483 dense core. |
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| Contributor(s): H. S. P. Müller; 05, 2015 | Contributor(s): H. S. P. Müller; 05, 2015 |
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