2024-03-29T13:40:55Zhttp://uvadoc.uva.es/oai/requestoai:uvadoc.uva.es:10324/226312021-06-23T11:52:51Zcom_10324_1186com_10324_931com_10324_894col_10324_1404
Laboratory characterization and astrophysical detection of vibrationally excited states of vinyl cyanide in Orion-KL
López, A.
Tercero, Belen
Kisiel, Z.
Daly, Adam M.
Bermúdez 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
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.
2017-03-16T11:17:02Z
2017-03-16T11:17:02Z
2014
info:eu-repo/semantics/article
https://doi.org/10.1051/0004-6361/201423622
A&A 572, A44 (2014)
http://uvadoc.uva.es/handle/10324/22631
eng
info:eu-repo/semantics/restrictedAccess
ESO 2014
application/pdf
EDP Science