The evolutionary history of ultra-compact accreting binaries

Context. AM Canum Venaticorum (AM CVn) stars are ultra-compact binary systems composed of a white dwarf primary accreting from a hydrogen-deficient donor. They play a crucial role in astrophysics as potential progenitors of Type Ia supernovae and as laboratories for gravitational wave studies. Howev...

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Bibliografiske detaljer

Principais autores:	Yu W., Pala A. F., Kupfer T., Gänsicke B. T., Koester D., Belloni D., Wong T. L. S., Schreiber M. R., van Roestel J., Brown A. J., Waagen E. O., González-Carballo J.-L., Bednarz S., Bernacki K., De Martino D., Fernández Mañanes E., González Farfán R., Green M. J., Groot P. J., Hambsch F.-J, Knigge C., Martin-Velasco J.-L., Morales-Aimar M., Myers G., Naves Nogues R., Poggiani R., Popowicz A., Ramsay G., Reina-Lorenz E., Rodríguez-Gil P., Salto-González J.-L., Sion E. M., Steeghs D., Szkody P., Toloza O., Tovmassian G.
Format:	Artigo
Sprog:	Inglês
Udgivet:	EDP Sciences 2026-02-01
Serier:	Astronomy & Astrophysics
Fag:	stars: atmospheres binaries: eclipsing binaries: spectroscopic novae cataclysmic variables white dwarfs
Online adgang:	https://www.aanda.org/articles/aa/full_html/2026/02/aa57568-25/aa57568-25.html
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