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...

Full description

Bibliographic Details
Authors: 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.
Format: article
Status:Published version
Publication Date:2022
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/296928
Online Access:http://hdl.handle.net/10261/296928
Access Level:Open access
Keyword:Galaxies: spiral
Galaxies: starburst
Masers
Submillimeter: galaxies
Radio lines: galaxies
Description
Summary:[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.

Similar Items