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20212024
most citedBrightness and mass accretion rate evolution during the 2022 burst of EX~Lupi

20 citations · 61 across the 7 of their papers we have counts for

collaborators

7 papers

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.HE2023

SN 2021gno: a Calcium-rich transient with double-peaked light curves

K. Ertini, G. Folatelli, L. Martinez +52

We present extensive ultraviolet (UV) and optical photometric and optical spectroscopic follow-up of supernova (SN)~2021gno by the "Precision Observations of Infant Supernova Explo…

astro-ph.SR202320 cited

Brightness and mass accretion rate evolution during the 2022 burst of EX~Lupi

F. Cruz-Sáenz de Miera, Á. Kóspál, P. Ábrahám +18

EX Lupi is the prototype by which EXor-type outbursts were defined. It has experienced multiple accretion-related bursts and outbursts throughout the last decades, whose study have…

astro-ph.SR202314 cited

Gaia21bty: An EXor lightcurve exhibiting an FUor spectrum

Michał Siwak, Lynne A. Hillenbrand, Ágnes Kóspál +16

Gaia21bty, a pre-main sequence star that previously had shown aperiodic dips in its light curve, underwent a considerable mag brightening that occurred over a few mo…

astro-ph.SR20234 cited

The Effelsberg survey of FU Orionis and EX Lupi objects I. -- Host environments of FUors/EXors traced by NH

Zs. M. Szabó, Y. Gong, K. M. Menten +6

FU Orionis (FUor) and EX Lupi (EXor) type objects represent two small, but rather spectacular groups of low-mass, young eruptive stars. Outbursts of several magnitudes are observed…

astro-ph.SR20225 cited

Photometric and spectroscopic study of the burst-like brightening of two Gaia-alerted young stellar objects

Zsófia Nagy, Péter Ábrahám, Ágnes Kóspál +18

Young stars show variability on different time-scales from hours to decades, with a range of amplitudes. We studied two young stars, which triggered the Gaia Science Alerts system…