Chemical tracers of a highly eccentric AGB–main-sequence star binary

Danilovich, T., Malfait, J., Van de Sande, M. et al. (32 more authors) (2024) Chemical tracers of a highly eccentric AGB–main-sequence star binary. Nature Astronomy, 8. pp. 308-327. ISSN 2397-3366

Abstract

Metadata

Item Type: Article
Authors/Creators:
  • Danilovich, T.
  • Malfait, J.
  • Van de Sande, M.
  • Montarges, M.
  • Kervella, P.
  • De Ceuster, F.
  • Coenegrachts, A.
  • Millar, T.J.
  • Richards, A.M.S.
  • Decin, L.
  • Gottlieb, C.A.
  • Pinte, C.
  • De Beck, E.
  • Price, D.J.
  • Wong, K.T.
  • Bolte, J.
  • Menten, K.M.
  • Baudry, A.
  • de Koter, A.
  • Etoka, S.
  • Gobrecht, D.
  • Gray, M.
  • Herpin, F.
  • Jeste, M.
  • Lagadec, E.
  • Maes, S.
  • McDonald, I.
  • Marinho, L.
  • Muller, H.S.P.
  • Pimpanuwat, B.
  • Plane, J. ORCID logo https://orcid.org/0000-0003-3648-6893
  • Sahai, R.
  • Wallstrom, S.H.J.
  • Yates, J.
  • Zijlstra, A.
Copyright, Publisher and Additional Information:

© The Author(s), under exclusive licence to Springer Nature Limited 2023. This version of the article has been accepted for publication, after peer review (when applicable) and is subject to Springer Nature’s AM terms of use (https://www.springernature.com/gp/open-research/policies/accepted-manuscript-terms), but is not the Version of Record and does not reflect post-acceptance improvements, or any corrections. The Version of Record is available online at: https://doi.org/10.1038/s41550-023-02154-y.
Dates:
  • Published: March 2024
  • Published (online): 3 January 2024
  • Accepted: 30 October 2023
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: 10 Oct 2023 11:52
Last Modified: 09 Oct 2024 14:57
Status: Published
Publisher: Nature Research
Identification Number: 10.1038/s41550-023-02154-y
Related URLs:
Open Archives Initiative ID (OAI ID):

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