Modelling predicts a molecule-rich disk around the AGB star L₂ Puppis

Van de Sande, M. orcid.org/0000-0001-9298-6265, Walsh, C. orcid.org/0000-0001-6078-786X, Danilovich, T. orcid.org/0000-0002-1283-6038 et al. (2 more authors) (2024) Modelling predicts a molecule-rich disk around the AGB star L₂ Puppis. Monthly Notices of the Royal Astronomical Society, 532 (1). pp. 734-754. ISSN 0035-8711

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Item Type: Article
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Copyright, Publisher and Additional Information:

© 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
Keywords: astrochemistry, molecular processes, radiative transfer, stars: AGB and post-AGB, circumstellar matter, stars: individual: HD 56096, L₂ Puppis
Dates:
  • Published: July 2024
  • Published (online): 21 June 2024
  • Accepted: 18 June 2024
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Funding Information:
Funder
Grant number
STFC (Science and Technology Facilities Council)
ST/X001016/1
EU - European Union
882991
MRC (Medical Research Council)
MR/T040726/1
Depositing User: Symplectic Publications
Date Deposited: 08 Jul 2024 09:24
Last Modified: 08 Jul 2024 09:24
Published Version: https://academic.oup.com/mnras/article/532/1/734/7...
Status: Published
Publisher: Oxford University Press (OUP)
Identification Number: 10.1093/mnras/stae1553
Open Archives Initiative ID (OAI ID):

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