QR Code

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...

Whakaahuatanga katoa

I tiakina i:
Ngā kaituhi matua: 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.
Hōputu: Artigo
Reo:Inglês
I whakaputaina: EDP Sciences 2026-02-01
Rangatū:Astronomy & Astrophysics
Ngā marau:
stars: atmospheres
binaries: eclipsing
binaries: spectroscopic
novae
cataclysmic variables
white dwarfs
Urunga tuihono:https://www.aanda.org/articles/aa/full_html/2026/02/aa57568-25/aa57568-25.html
Ngā Tūtohu: Tāpirihia he Tūtohu
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!

Ngā tūemi rite