Most extremely low mass white dwarfs with non-degenerate companions are inner binaries of hierarchical triples

Lagos-Vilches, F., Hernandez, M. orcid.org/0000-0001-5103-2713, Schreiber, M.R. orcid.org/0000-0003-3903-8009 et al. (2 more authors) (2024) Most extremely low mass white dwarfs with non-degenerate companions are inner binaries of hierarchical triples. Monthly Notices of the Royal Astronomical Society, 534 (4). pp. 3229-3236. ISSN 0035-8711

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Item Type: Article
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© 2024 The author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License ( https:// creativecommons.org/ licenses/ by/ 4.0/ ), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

Keywords: binaries (including multiple): close; stars: evolution; white dwarfs
Dates:
  • Published: November 2024
  • Published (online): 8 October 2024
  • Accepted: 2 October 2024
  • Submitted: 21 June 2024
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematical and Physical Sciences
Depositing User: Symplectic Sheffield
Date Deposited: 25 Oct 2024 11:23
Last Modified: 25 Oct 2024 11:23
Status: Published
Publisher: Oxford University Press (OUP)
Refereed: Yes
Identification Number: 10.1093/mnras/stae2310
Open Archives Initiative ID (OAI ID):

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