Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions - spherically symmetric ionized accretion flows

Lund, K, Wood, K, Falceta-Goncalves, D et al. (5 more authors) (2019) Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions - spherically symmetric ionized accretion flows. Monthly Notices of the Royal Astronomical Society, 485 (3). pp. 3761-3770. ISSN 0035-8711

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Copyright, Publisher and Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
Keywords: hydrodynamics; radiative transfer; stars: formation; stars: massive; H II regions
Dates:
  • Published: May 2019
  • Accepted: 28 February 2019
  • Published (online): 2 March 2019
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: 21 Aug 2019 11:28
Last Modified: 22 Aug 2019 04:19
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stz621
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