Symbiotic Star T CrB as an Extreme SU UMa–type Dwarf Nova

Symbiotic Star T CrB as an Extreme SU UMa–type Dwarf Nova

T CrB is a symbiotic recurrent nova that exhibits quiescent and active phases between its classical nova eruptions. The statistical properties of these active phases have been poorly studied thus far. Because of that their nature remained unknown. Here we study statistical properties of the active p...

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Bibliographic Details
Main Authors: Krystian Iłkiewicz, Joanna Mikołajewska, Kiril A. Stoyanov
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Dwarf novae
Classical novae
SU Ursae Majoris stars
Symbiotic binary stars
Online Access:https://doi.org/10.3847/2041-8213/ace9dc

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