Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs

Pala, A.F., Gänsicke, B.T., Belloni, D. et al. (28 more authors) (2022) Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs. Monthly Notices of the Royal Astronomical Society, 510 (4). pp. 6110-6132. ISSN 0035-8711

Abstract

Metadata

Item Type: Article
Authors/Creators:
  • Pala, A.F.
  • Gänsicke, B.T.
  • Belloni, D.
  • Parsons, S.G. ORCID logo https://orcid.org/0000-0002-2695-2654
  • Marsh, T.R.
  • Schreiber, M.R.
  • Breedt, E.
  • Knigge, C.
  • Sion, E.M.
  • Szkody, P.
  • Townsley, D.
  • Bildsten, L.
  • Boyd, D.
  • Cook, M.J.
  • De Martino, D.
  • Godon, P.
  • Kafka, S.
  • Kouprianov, V.
  • Long, K.S.
  • Monard, B.
  • Myers, G.
  • Nelson, P.
  • Nogami, D.
  • Oksanen, A.
  • Pickard, R.
  • Poyner, G.
  • Reichart, D.E.
  • Perez, D.R.
  • Shears, J.
  • Stubbings, R.
  • Toloza, O.
Copyright, Publisher and Additional Information:

© 2021 The Author(s). 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: stars: white dwarfs; cataclysmic variables; evolution; fundamental parameters
Dates:
  • Published: March 2022
  • Published (online): 27 November 2021
  • Accepted: 17 November 2021
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Funding Information:
Funder
Grant number
Science and Technology Facilities Council
ST/R003424/1
Depositing User: Symplectic Sheffield
Date Deposited: 13 Dec 2021 14:06
Last Modified: 16 Mar 2022 10:10
Status: Published
Publisher: Oxford University Press (OUP)
Refereed: Yes
Identification Number: 10.1093/mnras/stab3449
Related URLs:
Open Archives Initiative ID (OAI ID):

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