47 citations · 184 across the 10 of their papers we have counts for
10 papers
Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds
F. D. Priestley, P. C. Clark, S. C. O. Glover +4
Much of what we know about molecular clouds, and by extension star formation, comes from molecular line observations. Interpreting these correctly requires knowledge of the underly…
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…