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

Homan, W, Pimpanuwat, B, Herpin, F et al. (36 more authors) (2021) 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. Astronomy and Astrophysics, 651. A82. ISSN 0004-6361

Abstract

Metadata

Authors/Creators:
  • Homan, W
  • Pimpanuwat, B
  • Herpin, F
  • Danilovich, T
  • McDonald, I
  • Wallström, SHJ
  • Richards, AMS
  • Baudry, A
  • Sahai, R
  • Millar, TJ
  • Koter, AD
  • Gottlieb, CA
  • Kervella, P
  • Montargès, M
  • Van de Sande, M
  • Decin, L
  • Zijlstra, A
  • Etoka, S
  • Jeste, M
  • Müller, HSP
  • Maes, S
  • Malfait, J
  • Menten, K
  • Plane, J ORCID logo https://orcid.org/0000-0003-3648-6893
  • Lee, K
  • Waters, R
  • Wong, KT
  • Lagadec, E
  • Gobrecht, D
  • Yates, J
  • Price, D
  • Cannon, E
  • Bolte, J
  • De Ceuster, F
  • Nuth, J
  • Sindel, JP
  • Kee, D
  • Gray, MD
  • El Mellah, I
Copyright, Publisher and Additional Information: © ESO 2021. This is an author produced version of an article published in Astronomy and Astrophysics. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: stars: AGB and post-AGB; circumstellar matter; submillimeter: stars
Dates:
  • Published: July 2021
  • Accepted: 25 March 2021
  • Published (online): 20 July 2021
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Chemistry (Leeds) > Physical Chemistry (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 01 Apr 2021 10:14
Last Modified: 24 Jul 2021 14:26
Status: Published
Publisher: EDP Sciences
Identification Number: https://doi.org/10.1051/0004-6361/202140512

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