On the origin of the correlations between the accretion luminosity and emission line luminosities in pre-main-sequence stars

Mendigutia, I, Oudmaijer, RD, Rigliaco, E et al. (5 more authors) (2015) On the origin of the correlations between the accretion luminosity and emission line luminosities in pre-main-sequence stars. Monthly Notices of the Royal Astronomical Society, 452 (3). pp. 2837-2844. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • Mendigutia, I
  • Oudmaijer, RD
  • Rigliaco, E
  • Fairlamb, JR
  • Calvet, N
  • Muzerolle, J
  • Cunningham, N
  • Lumsden, SL
Copyright, Publisher and Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: accretion, accretion discs; line: formation; methods: miscellaneous; stars: pre-main sequence; stars: variables: T Tauri, Herbig Ae/Be
Dates:
  • Published: 21 September 2015
  • Accepted: 8 July 2015
  • Published (online): 29 July 2015
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: 30 Mar 2016 12:40
Last Modified: 30 Mar 2016 12:40
Published Version: http://dx.doi.org/10.1093/mnras/stv1540
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stv1540
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