activity
20222026
most citedA multi-epoch, multi-wavelength study of the classical FUor V1515 Cyg approaching quiescence

18 citations · 45 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026

Fast and furious -- High-velocity features of Ca and Si in the spectra of Type Ia supernovae

Zsófia Bora, József Vinkó, J. Craig Wheeler +2

High velocity absorption lines of Ca II and Si II (high-velocity features, HVFs) are common in the early spectra of Type Ia supernovae (SNe Ia), but their physical origin is still…

astro-ph.SR2026

SN 2026dix: a nearby, transitional Type IIb/Ib supernova consistent with a warm supergiant progenitor

Tamás Szalai, Schuyler D. Van Dyk, Dominik Bánhidi +20

Understanding the final evolution stages of (very) massive stars and their explosive outcomes, stripped-envelope supernovae (SESNe), represent a long-term challenge for astrophysic…

astro-ph.SR2026

The FU Ori outburst of PR Ori B

Carlos Contreras Pena, Zsofia Nagy, Gregory Herczeg +42

We report the discovery of a nearby FU Ori-type outburst (FUor), PR Ori B, in the L1641 cluster of the Orion star-forming region. The high-amplitude variability was first identifie…

astro-ph.HE2026

Long-term optical and near-infrared photometric evolution of SN 2019vxm, an interacting Type IIn supernova

Klára Lelkes, László Molnár, József Vinkó +12

The diversity of Type IIn supernovae is largely driven by the properties of the circumstellar material (CSM) they explode into. We examine the temporal evolution of SN 2019vxm, an…

astro-ph.EP2025★ 2 cited

NEO and imminent impactor discoveries from Hungary: recent results and lessons learnt

Norton O. Szabo, Krisztian Sarneczky, Laszlo L. Kiss +15

2022 EB5, 2023 CX1 and 2024 BX1: these are the three recent imminent impactor discoveries from the Piszkéstető Mountain Station of the Konkoly Observatory. They make up about one p…

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★ 4 cited

Short- and long-term variations of the high mass accretion rate classical T Tauri star DR Tau

Gabriella Zsidi, Ágnes Kóspál, Péter Ábrahám +20

Classical T Tauri stars are newly formed, low mass stars which may display both periodic and random variations in their brightness. The interaction between the star and its circums…

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.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★ 5 cited

The Enigma of Gaia18cjb: a Rare Hybrid of FUor and EXor?

Eleonora Fiorellino, Peter Abraham, Agnes Kospal +28

Context. Gaia18cjb is one of the Gaia-alerted eruptive young star candidates which has been experiencing a slow and strong brightening during the last 13 years, similar to some FU…

astro-ph.SR2023★ 7 cited

Three is the magic number -- distance measurement of NGC 3147 using SN 2021hpr and its siblings

Barnabas Barna, Andrea P. Nagy, Zsofia Bora +15

The nearby spiral galaxy NGC 3147 hosted three Type Ia supernovae (SNe Ia) in the past decades, which have been subjects of intense follow-up observations. Simultaneous analysis of…

astro-ph.SR2023★ 9 cited

Initial 56Ni Masses in Type Ia Supernovae

Zsófia Bora, József Vinkó, Réka Könyves-Tóth

We infer initial masses of the synthesized radioactive nickel-56 in a sample of recent Type Ia supernovae applying a new formalism introduced recently by Khatami & Kasen (2019). It…

astro-ph.SR2022★ 18 cited

A multi-epoch, multi-wavelength study of the classical FUor V1515 Cyg approaching quiescence

Zs. M. Szabó, Á. Kóspál, P. Ábrahám +28

Historically, FU Orionis-type stars are low-mass, pre-main sequence stars. The members of this class experience powerful accretion outbursts and remain in an enhanced accretion sta…