most citedOn the incidence rate of RR Lyrae stars with non-radial modes

4 citations · 4 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2025

SN 2023ixf in M101: physical parameters from bolometric light curve modeling

J. Vinko, Zs. R. Bodola, A. Godeny +25

We present new photometric observations of the core-collapse supernova SN 2023ixf occurred in M101, taken with the RC80 and BRC80 robotic telescopes in Hungary. The initial nickel…

astro-ph.SR2025

The 2023 outburst of the Gaia alerted EXor Gaia23bab

Zsófia Nagy, Ágnes Kóspál, Péter Ábrahám +33

Episodic accretion is a fundamental process in the build-up of the stellar mass. EX Lupi-type eruptive young stars (EXors) represent one of the main types of episodic accretion. We…

astro-ph.SR2025

Search for binary-channel metal-rich RR~Lyrae candidates

Hedieh Abdollahi, László Molnár, Vázsony Varga

The existence of dynamically young and metal-rich RR Lyrae stars challenges conventional notions of these variable stars. One possible scenario for their formation and evolution is…

astro-ph.HE2024

Ejecta masses in Type Ia Supernovae -- Implications for the Progenitor and the Explosion Scenario

Zsófia Bora, Réka Könyves-Tóth, József Vinkó +35

The progenitor system(s) as well as the explosion mechanism(s) of thermonuclear (Type Ia) supernovae are long-standing issues in astrophysics. Here we present ejecta masses and oth…

astro-ph.SR2024★ 4 cited

On the incidence rate of RR Lyrae stars with non-radial modes

H. Netzel, V. Varga, R. Szabo +2

Over the recent years, additional low-amplitude non-radial modes were detected in many of the first-overtone RR Lyrae stars. These non-radial modes form a characteristic period rat…