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Sporadic radio pulses from a white dwarf binary at the orbital period

ILT J1101 is a white dwarf–M dwarf binary that emits minute-duration radio pulses with a 2-h periodicity. The period of the radio pulses is linked to the orbital period of the binary, rather than the rotation period of the stellar components.

I. de Ruiter
K. M. Rajwade
S. Mahadevan
ResearchOpen Access12 Mar 2025
Nature Astronomy

Volume: 9, P: 672-684
Publisher Correction: Sporadic radio pulses from a white dwarf binary at the orbital period

I. de Ruiter
K. M. Rajwade
S. Mahadevan
Amendments and CorrectionsOpen Access01 Apr 2025
Nature Astronomy

Volume: 9, P: 747
A giant planet candidate transiting a white dwarf

A giant planet candidate roughly the size of Jupiter but more than 14 times as massive is observed by TESS and other instruments to be transiting the white dwarf star WD 1856+534.

Andrew Vanderburg
Saul A. Rappaport
Liang Yu
Research16 Sept 2020
Nature

Volume: 585, P: 363-367

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Sporadic radio pulses from a white dwarf binary at the orbital period

Publisher Correction: Sporadic radio pulses from a white dwarf binary at the orbital period

A giant planet candidate transiting a white dwarf

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