47 citations · 184 across the 10 of their papers we have counts for
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An APEX study of molecular outflows in FUor-type stars
Fernando Cruz-Sáenz de Miera, Ágnes Kóspál, Péter Ábrahám +4
FU Orionis-type objects (FUors) are low-mass pre-main-sequence objects which go through a short-lived phase (~100 years) of increased mass accretion rate (from 10^-8 to 10^-4 M_sun…
The first radio spectrum of a rapidly rotating A-type star
Jacob Aaron White, F. Tapia-Vázquez, A. G. Hughes +9
The radio spectra of main-sequence stars remain largely unconstrained due to the lack of observational data to inform stellar atmosphere models. As such, the dominant emission mech…
Episodic accretion in focus: revealing the environment of FU Orionis-type stars
O. Fehér, Á. Kóspál, P. Ábrahám +3
The earliest phases of star formation are characterised by intense mass accretion from the circumstellar disk to the central star. One group of young stellar objects, the FU Orioni…
A Study of Millimeter Variability in FUor Objects
John Wendeborn, Catherine C. Espaillat, Enrique Macias +6
FU Orionis objects (FUors) are rapidly-accreting, pre-main sequence objects that are known to exhibit large outbursts at optical and near-infrared wavelengths, with post-eruption,…
Envelope-to-disk mass transport in the FUor-type young eruptive star V346 Normae
Á. Kóspál, P. Ábrahám, O. Fehér +2
Having disk-to-star accretion rates on the order of 10/yr, FU Orionis-type stars (FUors) are thought to be the visible examples for episodic accretion. FUors are…