A primordial origin for molecular oxygen in comets: a chemical kinetics study of the formation and survival of O₂ ice from clouds to discs

Taquet, V, Furuya, K, Walsh, C orcid.org/0000-0001-6078-786X et al. (1 more author) (2016) A primordial origin for molecular oxygen in comets: a chemical kinetics study of the formation and survival of O₂ ice from clouds to discs. Monthly Notices of the Royal Astronomical Society, 462 (Suppl 1). S99-S115. ISSN 0035-8711

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Copyright, Publisher and Additional Information: © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: astrochemistry; comets: individual: 67P/C-G; protoplanetary discs; stars: formation; ISM: abundances; ISM: molecules
Dates:
  • Published: 16 November 2016
  • Accepted: 25 August 2016
  • Published (online): 2 September 2016
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)
Depositing User: Symplectic Publications
Date Deposited: 08 Nov 2016 11:57
Last Modified: 08 Nov 2016 11:57
Published Version: https://doi.org/10.1093/mnras/stw2176
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stw2176

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