33 citations · 78 across the 4 of their papers we have counts for
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Radiative Transfer modeling of EC 53: An Episodically Accreting Class I Young Stellar Object
Giseon Baek, Benjamin A. MacFarlane, Jeong-Eun Lee +8
In the episodic accretion scenario, a large fraction of the protostellar mass accretes during repeated and large bursts of accretion. Since outbursts on protostars are typically id…
Observational signatures of outbursting protostars -- II: Exploring a wide range of eruptive protostars
Benjamin MacFarlane, Dimitris Stamatellos, Doug Johnstone +5
Young stars exhibit variability due to changes in the gas accretion rate onto them, an effect that should be quite significant in the early stages of their formation. As protostars…
Observational signatures of outbursting protostars - I: From hydrodynamic simulations to observations
Benjamin MacFarlane, Dimitris Stamatellos, Doug Johnstone +5
Accretion onto protostars may occur in sharp bursts. Accretion bursts during the embedded phase of young protostars are probably most intense, but can only be inferred indirectly t…
The structure of young embedded protostellar discs
Benjamin A. MacFarlane, Dimitris Stamatellos
Young protostellar discs provide the initial conditions for planet formation. The properties of these discs may be different from those of late-phase (T Tauri) discs due to continu…