Evolution of Chemistry in the envelope of HOt CorinoS (ECHOS) II. The puzzling chemistry of isomers as revealed by the HNCS/HSCN ratio

[Context] The observational detection of some metastable isomers in the interstellar medium with abundances comparable to those of the most stable isomer, or even when the stable isomer is not detected, highlights the importance of non-equilibrium chemistry. This challenges our understanding of the...

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Detalles Bibliográficos
Autores: Esplugues, Gisela, Rodríguez-Baras, M., Navarro-Almaida, David, Fuente, Asunción, Fernández-Ruiz, Patricia, Spezzano, S., Drozdovskaya, M. N., Sánchez-Monge, Álvaro, Caselli, Paola, Riviere-Marichalar, Pablo, Beitia-Antero, L.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/382102
Acceso en línea:http://hdl.handle.net/10261/382102
Access Level:acceso abierto
Palabra clave:ISM: abundances
ISM: clouds
ISM: molecules
Descripción
Sumario:[Context] The observational detection of some metastable isomers in the interstellar medium with abundances comparable to those of the most stable isomer, or even when the stable isomer is not detected, highlights the importance of non-equilibrium chemistry. This challenges our understanding of the interstellar chemistry and shows the need to study isomeric forms of molecular species to constrain chemical processes occurring in the interstellar medium.