2026-04-27T14:37:43Zhttps://uvadoc.uva.es/oai/request

oai:uvadoc.uva.es:10324/226312025-03-04T09:45:54Zcom_10324_1186com_10324_931com_10324_894col_10324_1404

López, A. Tercero, Belén Kisiel, Z. Daly, Adam M. Bermudez Arias, María Celina Calcutt, H. Marcelino, N. Viti, S. Drouin, B. J. Medveded, I.R. Neese, C.F. Pszczółkowski, L. Alonso Hernández, José Luis Cernicharo, José 2017-03-16T11:17:02Z 2017-03-16T11:17:02Z 2014 A&A 572, A44 (2014) http://uvadoc.uva.es/handle/10324/22631 10.1051/0004-6361/201423622 We perform a laboratory characterization in the 18–1893 GHz range and astronomical detection between 80–280 GHz in Orion-KL with IRAM-30 m of CH2CHCN (vinyl cyanide) in its ground and vibrationally excited states. Aims: Our aim is to improve the understanding of rotational spectra of vibrationally excited vinyl cyanide with new laboratory data and analysis. The laboratory results allow searching for these excited state transitions in the Orion-KL line survey. Furthermore, rotational lines of CH2CHCN contribute to the understanding of the physical and chemical properties of the cloud. eng info:eu-repo/semantics/restrictedAccess ESO 2014 Laboratory characterization and astrophysical detection of vibrationally excited states of vinyl cyanide in Orion-KL info:eu-repo/semantics/article