Unveiling the white dwarf in J191213.72 − 441045.1 through ultraviolet observations

ABSTRACT J191213.72 − 441045.1 is a binary system composed of a white dwarf and an M-dwarf in a 4.03-h orbit. It shows emission in radio, optical, and X-ray, all modulated at the white dwarf spin period of 5.3 min, as well as various orbital sideband frequencies. Like in the prototype of the class o...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2024-01, Vol.527 (2), p.3826-3836
Hauptverfasser:	Pelisoli, Ingrid, Sahu, Snehalata, Lyutikov, Maxim, Barkov, Maxim, Gänsicke, Boris T, Brink, Jaco, Buckley, David A H, Potter, Stephen B, Schwope, Axel, Ramírez, S H
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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