ATOMIUM: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae I. Morpho-kinematical interpretation of CO and SiO emission (2021)
Attributed to:
Queen's University Belfast Astronomy Observation and Theory Consolidated Grant 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202140512
Publication URI: http://dx.doi.org/10.1051/0004-6361/202140512
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics