Methanol formation in TW Hya and future prospects for detecting larger complex molecules in disks with ALMA

Walsh, C orcid.org/0000-0001-6078-786X, Vissapragada, S and McGee, H (2018) Methanol formation in TW Hya and future prospects for detecting larger complex molecules in disks with ALMA. Proceedings of the International Astronomical Union, 13. pp. 395-402. ISSN 1743-9213

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Copyright, Publisher and Additional Information: © 2018, International Astronomical Union. This article has been published in a revised form in Proceedings of the International Astronomical Union https:// doi.org/10.1017/S1743921317007037. This version is free to view and download for private research and study only. Not for re-distribution, re-sale or use in derivative works. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: astrochemistry; planetary systems: protoplanetary disks; molecular processes; stars: individual (TW Hya)
Dates:
  • Published: 4 September 2018
  • Accepted: 6 September 2017
  • Published (online): 4 September 2018
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: 03 May 2018 10:42
Last Modified: 04 Mar 2019 01:39
Status: Published
Publisher: Cambridge University Press
Identification Number: https://doi.org/10.1017/S1743921317007037

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