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| dc.contributor.author | López, A. | |
| dc.contributor.author | Tercero, Belen | |
| dc.contributor.author | Kisiel, Z. | |
| dc.contributor.author | Daly, Adam M. | |
| dc.contributor.author | Bermúdez Arias, María Celina | |
| dc.contributor.author | Calcutt, H. | |
| dc.contributor.author | Marcelino, N. | |
| dc.contributor.author | Viti, S. | |
| dc.contributor.author | Drouin, B. J. | |
| dc.contributor.author | Medveded, I.R. | |
| dc.contributor.author | Neese, C.F. | |
| dc.contributor.author | Pszczółkowski, L. | |
| dc.contributor.author | Alonso Hernández, José Luis | |
| dc.contributor.author | Cernicharo, José | |
| dc.date.accessioned | 2017-03-16T11:17:02Z | |
| dc.date.available | 2017-03-16T11:17:02Z | |
| dc.date.issued | 2014 | |
| dc.identifier.citation | A&A 572, A44 (2014) | es |
| dc.identifier.uri | http://uvadoc.uva.es/handle/10324/22631 | |
| dc.description.abstract | 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. | es |
| dc.format.mimetype | application/pdf | es |
| dc.language.iso | eng | es |
| dc.publisher | EDP Science | es |
| dc.rights.accessRights | info:eu-repo/semantics/restrictedAccess | es |
| dc.title | Laboratory characterization and astrophysical detection of vibrationally excited states of vinyl cyanide in Orion-KL | es |
| dc.type | info:eu-repo/semantics/article | es |
| dc.rights.holder | ESO 2014 | es |
| dc.identifier.doi | 10.1051/0004-6361/201423622 | es |
| dc.peerreviewed | SI | es |
