Water masers high resolution measurements of the diverse conditions in evolved star winds

A. M.S. Richards, Y. Asaki, A. Baudry, J. Brand, L. Decin, S. Etoka, M. D. Gray, F. Herpin, R. Humphreys, B. Pimpanuwat, A. P. Singh, J. A. Yates, L. M. Ziurys

Research output: Contribution to journalArticlepeer-review

Abstract

We compare detailed observations of multiple H2O maser transitions around the red supergiant star VY CMa with models to constrain the physical conditions in the complex outflows. The temperature profile is consistent with a variable mass loss rate but the masers are mostly concentrated in dense clumps. High-excitation lines trace localised outflows near the star.

Original languageEnglish (US)
Pages (from-to)389-391
Number of pages3
JournalProceedings of the International Astronomical Union
Volume18
DOIs
StatePublished - Dec 7 2022

Keywords

  • Masers
  • Mass loss
  • Stars: massive

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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