37 citations · 55 across the 3 of their papers we have counts for
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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.SR2021★ 37 cited
Massive compact disks around FU Orionis-type young eruptive stars revealed by ALMA
Á. Kóspál, F. Cruz-Sáenz de Miera, J. A. White +14
FU Orionis-type objects (FUors) are low-mass pre-main sequence stars undergoing a temporary, but significant increase of mass accretion rate from the circumstellar disk onto the pr…