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--- molecules:ism:harnstoff [2020/11/06 12:24] – mueller
+++ molecules:ism:harnstoff [2020/11/06 12:59] (current) – mueller
@@ Line 7: / Line 7: @@
 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, L. Rodríguez-Almeida, E. R. Alonso Alonso, S. Zeng, E. J. Cocinero, S. Martín, M. Requena-Torres, R. Martín-Domenech, and L. Testi\\
-investigated\\
+reported on\\
-**[[https://doi.org/10.3847/1538-4357/abad38|The Family of Amide Molecules toward NGC 6334I]]**\\
+**[[https://doi.org/10.1089/ast.2019.2125|Toward the RNA-World in the Interstellar Medium − Detection of Urea and Search of 2-Aminooxazole and Simple Sugars]]**\\
-//Astrophys. J.// **901**, Art. No. 37 (2020).\\
+//Astrobiology// **20**, 1048−1066 (2020).\\
-They detected the molecule toward the position MM1-v.\\
+The molecule was detected in the course of n unbiased molecular line survey of the quiescent giant molecular cloud G+0.693−0.027, about 1' north-east of Sagittarius B2(N), with the IRAM 30 m dish at 3 and 2 mm.