A 5.3-min-period pulsing white dwarf in a binary detected from radio to X-rays-Reference-Cited by-同舟云学术

A 5.3-min-period pulsing white dwarf in a binary detected from radio to X-rays

Published:2023-06-15 Issue:8 Volume:7 Page:931-942
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Pelisoli Ingrid^ORCID,Marsh T. R.,Buckley David A. H.^ORCID,Heywood I.^ORCID,Potter Stephen. B.,Schwope Axel,Brink Jaco^ORCID,Standke Annie,Woudt P. A.,Parsons S. G.^ORCID,Green M. J.,Kepler S. O.^ORCID,Munday James,Romero A. D.,Breedt E.^ORCID,Brown A. J.^ORCID,Dhillon V. S.^ORCID,Dyer M. J.^ORCID,Kerry P.,Littlefair S. P.,Sahman D. I.^ORCID,Wild J. F.

Funder

RCUK | Science and Technology Facilities Council

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-023-01995-x.pdf

Reference76 articles.

1. Stanway, E. R. et al. VLA radio observations of AR Scorpii. Astron. Astrophys. 611, A66 (2018).

2. Takata, J. et al. A non-thermal pulsed X-ray emission of AR Scorpii. Astrophys. J. 853, 106 (2018).

3. Marsh, T. R. et al. A radio-pulsing white dwarf binary star. Nature 537, 374–377 (2016).

4. Katz, J. I. AR Sco: a precessing white dwarf synchronar? Astrophys. J. 835, 150 (2017).

5. Takata, J., Yang, H. & Cheng, K. S. A model for AR Scorpii: emission from relativistic electrons trapped by closed magnetic field lines of magnetic white dwarfs. Astrophys. J. 851, 143 (2017).

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