25 GHz methanol masers in regions of massive star formation

Tui R. Britton*, Maxim A. Voronkov

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution

Abstract

The bright 25 GHz series of methanol masers is formed in highly energetic regions of massive star formation and provides a natural signpost of shocked gas surrounding newly forming stars. A systematic survey for the 25 GHz masers has only recently been carried out. We present the preliminary results from the interferometric follow up of 51 masers at 25 GHz in the southern sky.

Original languageEnglish
Title of host publicationCosmic Masers - from OH to H0
EditorsRoy S. Booth, Elizabeth M. L. Humphreys, Wouter H. T. Vlemmings
Place of PublicationCambridge
PublisherCambridge University Press
Pages282-283
Number of pages2
Volume8
EditionS287
ISBN (Print)9781107032842
DOIs
Publication statusPublished - Jul 2012

Publication series

NameProceedings of the International Astronomical Union
NumberS287
Volume8
ISSN (Print)17439213
ISSN (Electronic)17439221

Fingerprint Dive into the research topics of '25 GHz methanol masers in regions of massive star formation'. Together they form a unique fingerprint.

  • Cite this

    Britton, T. R., & Voronkov, M. A. (2012). 25 GHz methanol masers in regions of massive star formation. In R. S. Booth, E. M. L. Humphreys, & W. H. T. Vlemmings (Eds.), Cosmic Masers - from OH to H0 (S287 ed., Vol. 8, pp. 282-283). (Proceedings of the International Astronomical Union; Vol. 8, No. S287). Cambridge: Cambridge University Press. https://doi.org/10.1017/S1743921312007144