Can variability account for apparent age spreads in OB association colour-magnitude diagrams?

Burningham, B., Naylor, T., Littlefair, S.P. orcid.org/0000-0001-7221-855X et al. (1 more author) (2005) Can variability account for apparent age spreads in OB association colour-magnitude diagrams? Monthly Notices of the Royal Astronomical Society, 363 (4). pp. 1389-1397. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © 2005 The Authors. Journal compilation © 2005 RAS. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: stars: formation; stars: low-mass, brown dwarfs; stars: pre-main-sequence; stars: variables: other; open clusters and associations: individual: σ Orionis; open clusters and associations: individual: Cep OB3b
Dates:
  • Accepted: 17 August 2005
  • Published (online): 11 November 2005
  • Published: 11 November 2005
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 10 Apr 2019 15:06
Last Modified: 10 Apr 2019 15:06
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1111/j.1365-2966.2005.09535.x

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