Reconstructing the shock history in the CMZ of NGC 253 with ALCHEMI

[Context] HNCO and SiO are well-known shock tracers and have been observed in nearby galaxies, including the nearby (D = 3.5 Mpc) starburst galaxy NGC 253. The simultaneous detection of these two species in regions where the star-formation rate is high may be used to study the shock history of the g...

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Detalles Bibliográficos
Autores: Huang, Ko-Yun, Viti, Serena, Holdship, Jonathan, Mangum, Jeffrey G., Martín, Sergio, Harada, Nanase, Müller, Sebastien, Sakamoto, Kazushi, Tanaka, Kunihito, Yoshimura, Yuki, Herrero-Illana, Rubén, Meier, David S., Behrens, Erica, Werf, Paul van der, Henkel, Christian, García-Burillo, Santiago, Rivilla, Víctor M., Emig, Kimberly L., Colzi, Laura, Humire, P. K., Aladro, Rebeca, Bouvier, Mathilde
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2023
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/348593
Acceso en línea:http://hdl.handle.net/10261/348593
Access Level:acceso abierto
Palabra clave:Galaxies: ISM
Galaxies: individual: NGC253
Astrochemistry
Galaxies: starburst
ISM: molecules
Descripción
Sumario:[Context] HNCO and SiO are well-known shock tracers and have been observed in nearby galaxies, including the nearby (D = 3.5 Mpc) starburst galaxy NGC 253. The simultaneous detection of these two species in regions where the star-formation rate is high may be used to study the shock history of the gas.

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