activity
20122026
most citedPlanet Hunters X. KIC 8462852 - Where's the Flux?

289 citations · 2k across the 88 of their papers we have counts for

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Showing 2022Show all

7 papers · 1 filter

astro-ph.SR2022

Surface activity of the G dwarf primary in the quaternary star system V815 Her

Zsolt Kővári, Klaus G. Strassmeier, Tamás Borkovits +4

We investigate the magnetic activity of the G dwarf primary star in the multiple system V815 Herculis. Recently, TESS Sector 26 data have revealed that V815 Her is in fact a four-s…

astro-ph.SR2022★ 18 cited

Photometric and spectroscopic study of the EXor-like eruptive young star Gaia19fct

Sunkyung Park, Ágnes Kóspál, Péter Ábrahám +19

Gaia19fct is one of the Gaia-alerted eruptive young stars that has undergone several brightening events. We conducted monitoring observations using multi-filter optical and near-in…

astro-ph.SR2022★ 6 cited

Mid-infrared time-domain study of recent dust production events in the extreme debris disc of TYC 4209-1322-1

A. Moór, P. Ábrahám, Á. Kóspál +23

Extreme debris discs are characterized by unusually strong mid-infrared excess emission, which often proves to be variable. The warm dust in these discs is of transient nature and…

astro-ph.SR2022★ 15 cited

Characteristics of flares on giant stars

Katalin Oláh, Bálint Seli, Zsolt Kővári +2

Although late-type dwarfs and giant stars are substantially different, their flares are thought to originate in similar physical processes and differ only by a scale factor in the…

astro-ph.SR2022★ 5 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…

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…

astro-ph.HE2022★ 21 cited

Probing into emission mechanisms of GRB 190530A using time-resolved spectra and polarization studies: Synchrotron Origin?

Rahul Gupta, S. Gupta, T. Chattopadhyay +47

Multi-pulsed GRB 190530A, detected by the GBM and LAT onboard \fermi, is the sixth most fluent GBM burst detected so far. This paper presents the timing, spectral, and polarimetric…