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--- molecules:ism:harnstoff [2019/07/26 15:45] – created mueller
+++ molecules:ism:harnstoff [2020/11/06 12:55] – mueller
@@ Line 5: / Line 5: @@
 **[[https://doi.org/10.1051/0004-6361/201935428|Re-exploring Molecular Complexity with ALMA (ReMoCA): Interstellar Detection of Urea]]**\\
 //Astron. Astrophys.// **628**, Art. No. A10 (2019).\\
+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).\\
+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\\
+reported on\\
+**[[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]]**\\
+//Astron. Astrophys.// **20**, 1048−1066 (2020).\\
+----
+Contributor(s): H. S. P. Müller; 07, 2019; 11, 2020
+----