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- | ===== On the Detection of Methyleneamodogen, H2CN, in the ISM ===== | + | ===== On the Detection of Methyleneamidogen, H2CN, in the ISM ===== |
M. Ohishi, D. McGonagle, W. M. Irvine, S. Yamamoto, and S. Saito\\ | M. Ohishi, D. McGonagle, W. M. Irvine, S. Yamamoto, and S. Saito\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[https:// | + | **[[https:// |
// | // | ||
+ | Two noisy features near 73.35 GHz, observed with the 12 m NRAO telescope at Kitt Peak, were assigned to < | ||
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+ | C. Vastel, J. C. Loison, V. Wakelam, and B. Lefloch\\ | ||
+ | reported on the\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | A molecular line survey of the prestellar core L1544 between 71.74 and 115.87 GHz was carried out with the IRAM 30 m telescope. Methyleneamidogen was observed through six hyperfine transitions around 73.4 GHz.\\ | ||
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+ | C. Cabezas, M. Agúndez, N. Marcelino, B. Tercero, S. Cuadrado, and J. Cernicharo\\ | ||
+ | reported on the\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | The authors give accounts on methyleneamidogen in the L483 and B1-b protostellar objects from earlier molecular line surveys carried out at 3 mm using the IRAM 30 m telescope; the L483 results were mentioned in an earlier publication, | ||
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+ | Contributor(s): | ||
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