Planet formation in intermediate-separation binary systems

Panić, O., Haworth, T.J., Petr-Gotzens, M.G. et al. (13 more authors) (2021) Planet formation in intermediate-separation binary systems. Monthly Notices of the Royal Astronomical Society, 501 (3). pp. 4317-4328. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • Panić, O.
  • Haworth, T.J.
  • Petr-Gotzens, M.G.
  • Miley, J.
  • van den Ancker, M.
  • Vioque, M.
  • Siess, L.
  • Parker, R.
  • Clarke, C.J.
  • Kamp, I.
  • Kennedy, G.
  • Oudmaijer, R.D.
  • Pascucci, I.
  • Richards, A.M.S.
  • Ratzka, T.
  • Qi, C.
Copyright, Publisher and Additional Information: © 2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. This is an author-produced version of a paper subsequently published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: planets and satellites: formation; protoplanetary discs; stars: pre-main-sequence; (stars:) binaries: visual; stars: variables: T Tauri, Herbig Ae/Be; submillimetre: planetary systems; techniques: interferometric
Dates:
  • Accepted: 27 November 2020
  • Published (online): 16 December 2020
  • Published: March 2021
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Funding Information:
FunderGrant number
ROYAL SOCIETYDH150108
Royal Society13178
Depositing User: Symplectic Sheffield
Date Deposited: 30 Mar 2021 12:48
Last Modified: 30 Mar 2021 12:48
Status: Published
Publisher: Oxford University Press (OUP)
Refereed: Yes
Identification Number: https://doi.org/10.1093/mnras/staa3834
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