collaborators
Showing astro-phShow all

9 papers · 1 filter

astro-ph200827 cited

The Challenge of Sub-Keplerian Rotation for Disk Winds

Frank H. Shu, Susana Lizano, Daniele Galli +2

Strong magnetization makes the disks surrounding young stellar objects rotate at rates that are too sub-Keplerian to enable the thermal launching of disk winds from their surfaces…

astro-ph2008108 cited

Monitoring the Large Proper Motions of Radio Sources in the Orion BN/KL Region

Laura Gomez, Luis F. Rodriguez, Laurent Loinard +4

We present absolute astrometry of four radio sources in the Becklin-Neugebauer/Kleinman-Low (BN/KL) region, derived from archival data (taken in 1991, 1995, and 2000) as well as fr…

astro-ph200714 cited

Formation of OB Associations in Galaxies

Frank H. Shu, Ronald J. Allen, Susana Lizano +1

We consider the formation of OB associations from two perspectives: (a) the fractional gas consumption in star formation,epsilon, per dynamical time scale t_dyn in a galaxy, and (b…

astro-ph200791 cited

Mean-Field Magnetohydrodynamics of Accretion Disks

Frank H. Shu, Daniele Galli, Susana Lizano +2

We consider the accretion process in a disk with magnetic fields that are dragged in from the interstellar medium by gravitational collapse. Two diffusive processes are at work in…

astro-ph200697 cited

Gravitational collapse of magnetized clouds II. The role of Ohmic dissipation

F. H. Shu, D. Galli, S. Lizano +1

We formulate the problem of magnetic field dissipation during the accretion phase of low-mass star formation, and we carry out the first step of an iterative solution procedure by…

astro-ph2006155 cited

Gravitational collapse of magnetized clouds. I. Ideal MHD accretion flow

D. Galli, S. Lizano, F. H. Shu +1

We study the self-similar collapse of an isothermal magnetized rotating cloud in the ideal magnetohydrodynamic (MHD) regime. In the limit of small distance from the accreting proto…