Planet formation in intermediate-separation binary systems

Panić, O, Haworth, TJ, Petr-Gotzens, MG 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, TJ
  • Petr-Gotzens, MG
  • Miley, J
  • van den Ancker, M
  • Vioque, M
  • Siess, L
  • Parker, R
  • Clarke, CJ
  • Kamp, I
  • Kennedy, G
  • Oudmaijer, RD ORCID logo https://orcid.org/0000-0001-7703-3992
  • Pascucci, I
  • Richards, AMS
  • 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 journal article 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 Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Funding Information:
FunderGrant number
STFC (Science and Technology Facilities Council)ST/P00041X/1
Royal SocietyDH140243
Depositing User: Symplectic Publications
Date Deposited: 15 Mar 2021 17:48
Last Modified: 15 Mar 2021 17:48
Status: Published
Publisher: Oxford University Press (OUP)
Identification Number: https://doi.org/10.1093/mnras/staa3834

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