Evidence of enhanced magnetism in cool, polluted white dwarfs

Author:

Kawka Adela1ORCID,Vennes Stéphane2,Ferrario Lilia2ORCID,Paunzen Ernst3ORCID

Affiliation:

1. International Centre for Radio Astronomy Research - Curtin University, GPO Box U1987, Perth, WA 6845, Australia

2. Mathematical Sciences Institute, The Australian National University, Canberra, ACT 0200, Australia

3. Department of Theoretical Physics and Astrophysics, Masaryk University, Kotlářská 2, CZ-611 37 Czech Republic

Funder

Czech Science Foundation

Australian National University

University of Western Australia

Uppsala University

University of Vienna

European School of Oncology

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 32 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The approximate coupled-cluster methods CC2 and CC3 in a finite magnetic field;The Journal of Chemical Physics;2024-03-05

2. Discovery of Magnetically Guided Metal Accretion onto a Polluted White Dwarf;The Astrophysical Journal Letters;2024-02-26

3. Rotation plays a role in the generation of magnetic fields in single white dwarfs;Monthly Notices of the Royal Astronomical Society;2024-01-31

4. A nearby polluted white dwarf with a 6.2 h spin period;Monthly Notices of the Royal Astronomical Society: Letters;2023-12-27

5. WD 0141−675: a case study on how to follow-up astrometric planet candidates around white dwarfs;Monthly Notices of the Royal Astronomical Society;2023-10-13

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