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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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