Blinded by the light: on the relationship between CO first overtone emission and mass accretion rate in massive young stellar objects

Ilee, JD, Oudmaijer, RD orcid.org/0000-0001-7703-3992, Wheelwright, HE et al. (1 more author) (2018) Blinded by the light: on the relationship between CO first overtone emission and mass accretion rate in massive young stellar objects. Monthly Notices of the Royal Astronomical Society, 477 (3). pp. 3360-3368. ISSN 0035-8711

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: This article has been published in Monthly Notices of the Royal Astronomical Society © 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: accretion, accretion discs; circumstellar matter; stars: formation; stars: massive; stars: pre-main-sequence
Dates:
  • Published: 1 July 2018
  • Accepted: 3 April 2018
  • Published (online): 5 April 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)
Funding Information:
FunderGrant number
PPARCST/F002092/1
Science & Technology Facilities Council (STFC)ST/L000628/1
Science & Technology Facilities Council (STFC)ST/P00041X/1
Depositing User: Symplectic Publications
Date Deposited: 25 May 2018 10:53
Last Modified: 25 May 2018 10:53
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/sty863

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