Methanol masers in NGC 253 with ALCHEMI

[Context] Methanol masers of Class I (collisionally pumped) and Class II (radiatively pumped) have been studied in great detail in our Galaxy in a variety of astrophysical environments such as shocks and star-forming regions and are they are helpful to analyze the properties of the dense interstella...

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Detalles Bibliográficos
Autores: Humire, P. K., Henkel, Christian, Hernández-Gómez, Antonio, Martín, Sergio, Mangum, Jeffrey G., Harada, Nanase, Müller, Sebastien, Herrero-Illana, Rubén, Meier, David S., Caux, Emmanuel, Aladro, Rebeca, Mauersberger, R., Viti, Serena, Colzi, Laura, Rivilla, Víctor M., Gorski, Mark, Menten, K. M., Huang, Ko-Yun, Aalto, Susanne, Werf, Paul van der, Emig, Kimberly L.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2022
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/296928
Acceso en línea:http://hdl.handle.net/10261/296928
Access Level:acceso abierto
Palabra clave:Galaxies: spiral
Galaxies: starburst
Masers
Submillimeter: galaxies
Radio lines: galaxies
Descripción
Sumario:[Context] Methanol masers of Class I (collisionally pumped) and Class II (radiatively pumped) have been studied in great detail in our Galaxy in a variety of astrophysical environments such as shocks and star-forming regions and are they are helpful to analyze the properties of the dense interstellar medium. However, the study of methanol masers in external galaxies is still in its infancy.

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