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A Jet Model of the Galactic Center Nonthermal Radio Filaments
F. Yusef-Zadeh, A. Königl
Protostellar sources in star forming regions are responsible for driving jets with flow velocities ranging between 300 and 400 km s. This class of jets consists of highly co…
The Formation and Early Evolution of Protostellar Accretion Disks
A. Konigl
Newly formed stars are often observed to possess circumstellar disks, from which mass continues to be accreted onto the star and fed into outflowing jets, and which eventually may…
The Supranova Model and Its Implications
Arieh Konigl
The supranova model for gamma-ray bursts, originally proposed by Vietri & Stella (1998), has several unique features that make it attractive for the interpretation of GRBs and thei…
Modeling Observational Signatures of Disk-Driven Outflows
J. E. Everett, A. Konigl, J. F. Kartje
We present a self-consistent, semi-analytical dynamical model of disk driven outflows in AGNs that are accelerated by a combination of magnetic stresses and radiation pressure. Thi…
Disk Winds and the Accretion--Outflow Connection
Arieh Konigl, Ralph E. Pudritz
We review recent observational and theoretical results on the relationship between circumstellar accretion disks and jets in young stellar objects. We then present a theoretical fr…