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Is the symbiotic recurrent nova T CrB late?
Jaroslav Merc, Łukasz Wyrzykowski, Paul G. Beck, P. J. Mikołajczyk, Krzysztof Kotysz, P. Zieliński, Staszek Zola, Mateusz Bronikowski, Jure Japelj, Matej Mihelčič
Izvirni znanstveni članek
Oznake: binaries;symbiotic;stars;T CrB;novae;cataclysmic variables;solar astrophysics;stellar astrophysics;high energy astrophysical phenomena;
T CrB is a symbiotic recurrent nova that last erupted in 1946. Given its recurrence time-scale of approximately 80 yr, the next outburst is eagerly anticipated by the astronomical community. In this work, we analyse the optical light curves of T CrB, comparing recent photometric evolution with histo ...
Leto: 2025 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
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