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molecules:ism:formamid [2019/05/09 12:38] – mueller | molecules:ism:formamid [2019/10/23 22:03] (current) – mueller | ||
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Formamide, HC(O)NH< | Formamide, HC(O)NH< | ||
R. H. Rubin, G. W. Swenson, Jr., R. C. Solomon, and H. L. Flygare,\\ | R. H. Rubin, G. W. Swenson, Jr., R. C. Solomon, and H. L. Flygare,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
They detected all three Δ// | They detected all three Δ// | ||
The detection of a second, related, 1 – 1 transition toward Sgr B2 and Sgr A was reported by\\ | The detection of a second, related, 1 – 1 transition toward Sgr B2 and Sgr A was reported by\\ | ||
C. A. Gottlieb, P. Palmer, L. J. Richard, and B. Zuckerman\\ | C. A. Gottlieb, P. Palmer, L. J. Richard, and B. Zuckerman\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
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//Astron. Astrophys.// | //Astron. Astrophys.// | ||
Carrying out a line survey toward IRAS 16293-2422 between 329 and 363 GHz, a deuteration degree of about two percent was derived for source B and for all three isotopomers assuming a < | Carrying out a line survey toward IRAS 16293-2422 between 329 and 363 GHz, a deuteration degree of about two percent was derived for source B and for all three isotopomers assuming a < | ||
+ | |||
+ | A. Belloche, R. T. Garrod, H. S. P. Müller, K. M. Menten, I. Medvedev, J. Thomas, and Z. Kisiel\\ | ||
+ | reported on\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | In the course of a new unbiased line survey toward the high-mass star-forming region Sagittarius (Sgr) B2(N) close to the Galactic center, HC(< | ||
The molecule was also detected in several other hot core sources, such as Orion KL, G327.3–0.6, | The molecule was also detected in several other hot core sources, such as Orion KL, G327.3–0.6, | ||
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Contributor(s): | Contributor(s): | ||
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