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molecules:ism:harnstoff [2020/11/06 12:24] – mueller | molecules:ism:harnstoff [2020/11/06 12:59] (current) – mueller | ||
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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).\\ | ||
- | N. F. W. Ligterink, S. J. El-Abd, C. L. Brogan, T. R. Hunter, A. J. Remijan, R. T. Garrod, and B. M. McGuire\\ | + | I. Jiménez-Serra, J. Martín-Pintado, V. M. Rivilla, |
- | investigated\\ | + | reported on\\ |
- | **[[https:// | + | **[[https:// |
- | //Astrophys. J.// **901**, Art. No. 37 (2020).\\ | + | //Astrobiology// **20**, 1048−1066 |
- | They detected the molecule toward | + | The molecule was detected |