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 language | English (US) |
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Pages (from-to) | 389-391 |
Number of pages | 3 |
Journal | Proceedings of the International Astronomical Union |
Volume | 18 |
DOIs | |
State | Published - Dec 7 2022 |
Keywords
- Masers
- Mass loss
- Stars: massive
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science