Precise mass and radius values for the white dwarf and low mass M dwarf in the pre-cataclysmic binary NN Serpentis

Parsons, S. G., Marsh, T. R., Copperwheat, C. M. et al. (4 more authors) (2010) Precise mass and radius values for the white dwarf and low mass M dwarf in the pre-cataclysmic binary NN Serpentis. Monthly Notices of the Royal Astronomical Society , 402 (4). pp. 2591-2608. ISSN 0035-8711

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2010 The Authors. This is an author produced version of a paper subsequently published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: binaries: eclipsing; stars: fundamental parameters; stars: individual: NN Ser; stars: late-type; white dwarfs
Dates:
  • Published: 1 March 2010
  • Accepted: 18 November 2009
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: 30 Nov 2016 16:59
Last Modified: 21 Mar 2018 00:50
Published Version: http://dx.doi.org/10.1111/j.1365-2966.2009.16072.x
Status: Published
Publisher: Oxford University Press (OUP): Policy P - Oxford Open Option A
Refereed: Yes
Identification Number: https://doi.org/10.1111/j.1365-2966.2009.16072.x

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