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dc.contributor.author | Alonso, E. R. | |
dc.contributor.author | Kolesniková, L. | |
dc.contributor.author | Tercero, B. | |
dc.contributor.author | Cabezas, C. | |
dc.contributor.author | Alonso, J. L. | |
dc.contributor.author | Cernicharo, J. | |
dc.contributor.author | Guillemin, J.-C. | |
dc.date.accessioned | 2024-02-08T11:09:55Z | |
dc.date.available | 2024-02-08T11:09:55Z | |
dc.date.issued | 2016 | |
dc.identifier.citation | The Astrophysical Journal, Volume 832, Number 1 | es |
dc.identifier.issn | 0004-637X | es |
dc.identifier.uri | https://uvadoc.uva.es/handle/10324/65989 | |
dc.description | Producción Científica | es |
dc.description.abstract | Previous detections of methyl and ethyl formate make other small substituted formates potential candidates for observation in the interstellar medium. Among them, vinyl formate is one of the simplest unsaturated carboxylic ester. The aim of this work is to provide direct experimental frequencies of the ground vibrational state of vinyl formate in a large spectral range for astrophysical use. The room-temperature rotational spectrum of vinyl formate has been measured from 80 to 360 GHz and analyzed in terms of Watson’s semirigid rotor Hamiltonian. Two thousand six hundred transitions within J = 3–88 and Ka = 0–28 were assigned to the most stable conformer of vinyl formate and a new set of spectroscopic constants was accurately determined. Spectral features of vinyl formate were then searched for in Orion KL, Sgr B2(N), B1-b, and TMC-1 molecular clouds. Upper limits to the column density of vinyl formate are provided. | es |
dc.format.mimetype | application/pdf | es |
dc.language.iso | spa | es |
dc.rights.accessRights | info:eu-repo/semantics/restrictedAccess | es |
dc.subject.classification | ISM: molecules – molecular data – techniques: spectroscopic | es |
dc.title | MILLIMETER WAVE SPECTRUM AND ASTRONOMICAL SEARCH FOR VINYL FORMATE | es |
dc.type | info:eu-repo/semantics/article | es |
dc.rights.holder | The American Astronomical Society | es |
dc.identifier.doi | 10.3847/0004-637X/832/1/42 | es |
dc.relation.publisherversion | https://iopscience.iop.org/article/10.3847/0004-637X/832/1/42 | es |
dc.identifier.publicationfirstpage | 42 | es |
dc.identifier.publicationissue | 1 | es |
dc.identifier.publicationtitle | The Astrophysical Journal | es |
dc.identifier.publicationvolume | 832 | es |
dc.peerreviewed | SI | es |
dc.description.project | European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC-2013-SyG, grant agreement No. 610256 NANOCOSMOS, Ministerio de Ciencia e Innovación (Grants CTQ2013-40717-P, AYA2012-32032, and Consolider-Ingenio 2010 CSD2009-00038 program "ASTROMOL"), and Junta de Castilla y León (grants VA070A08 and VA175U13), ANR-13-BS05-0008 IMOLABS | es |
dc.identifier.essn | 1538-4357 | es |
dc.type.hasVersion | info:eu-repo/semantics/draft | es |