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  5. Physical properties of Class I methanol masers
 

Physical properties of Class I methanol masers

Date Issued
2018
Author(s)
Leurini, Silvia  
•
Menten, Karl M.
DOI
10.1017/S1743921317010705
Abstract
As first realised in the late 1980s, methanol masers come in two varieties, termed Class I and Class II. While Class II masers had observationally been extensively studied in the past, until recently relatively little attention was paid to Class I methanol masers due to their low luminosities compared to other maser transitions. In this review, we will focus on the recent progress in our understanding of Class I methanol masers both from an observational and from a theoretical point of view.
Coverage
Astrophysical Masers: Unlocking the Mysteries of the Universe
All editors
Tarchi, Andrea; Reid, Mark J.; Castangia, Paola
Series
PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION  
Volume
vol. 13, S336
Start page
17
Conferenece
Astrophysical Masers: Unlocking the Mysteries of the Universe
Conferenece place
Cagliari, Italy
Conferenece date
4-8 September, 2017
Uri
http://hdl.handle.net/20.500.12386/28973
Url
https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/physical-properties-of-class-i-methanol-masers/5B42EAAD846BB017167A6100AAC77057
Issn Identifier
1743-9213
Ads BibCode
2018IAUS..336...17L
Rights
open.access
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physical_properties_of_class_i_methanol_masers.pdf

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