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molecules:ism:harnstoff [2019/07/26 16:23] – mueller | molecules:ism:harnstoff [2020/11/06 12:59] (current) – mueller | ||
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**[[https:// | **[[https:// | ||
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
- | Seven lines in the ground vibrational state and two lines in the lowest excited vibrational mode of urea were detected as unblended or marginally blended in the 3 mm wavelength region 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. The detections were made toward Sgr B2(N1S), a position about 1//"// south of the continuum peak of Sgr B2(N1). The molecule was not detected toward Sgr B2(N2). | + | Seven lines in the ground vibrational state and two lines in the lowest excited vibrational mode of urea were detected as unblended or marginally blended in the 3 mm wavelength region 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. The detections were made toward Sgr B2(N1S), a position about 1" south of the continuum peak of Sgr B2(N1). The molecule was not detected toward Sgr B2(N2).\\ |
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+ | I. Jiménez-Serra, | ||
+ | reported on\\ | ||
+ | **[[https:// | ||
+ | // | ||
+ | The molecule was detected in the course of n unbiased molecular line survey of the quiescent giant molecular cloud G+0.693−0.027, | ||
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- | Contributor(s): | + | Contributor(s): |
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