activity
19982011
most citedGravitational collapse of magnetized clouds II. The role of Ohmic dissipation

97 citations · 388 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2011★ 16 cited

Magnetic Interactions in Pre-Main-Sequence Binaries

Fred C. Adams, Michael J. Cai, Daniele Galli +2

Young stars typically have strong magnetic fields, so that the magnetospheres of newly formed close binaries can interact, dissipate energy, and produce synchrotron radiation. The…

astro-ph.GA2010★ 15 cited

Stability of Magnetized Disks and Implications for Planet Formation

Susana Lizano, Daniele Galli, Mike J. Cai +1

This paper considers gravitational perturbations in geometrically thin disks with rotation curves dominated by a central object, but with substantial contributions from magnetic pr…

astro-ph.SR2009★ 10 cited

The Equilibrium Structure of Prolate Magnetized Molecular Cores

Michael J. Cai, Ronald E. Taam

The structure of molecular cloud cores supported by thermal pressure and a poloidal magnetic field is reinvestigated in the magnetohydrostatic and axisymmetric approximation. In ad…

astro-ph.EP2009★ 36 cited

Migration of Extrasolar Planets: Effects from X-Wind Accretion Disks

Fred C. Adams, Mike J. Cai, Susana Lizano

Magnetic fields are dragged in from the interstellar medium during the gravitational collapse that forms star/disk systems. Consideration of mean field magnetohydrodynamics (MHD) i…

astro-ph.GA2009★ 30 cited

Polarized Emission of Sagittarius A*

Lei Huang, Siming Liu, Zhi-Qiang Shen +4

We explore the parameter space of the two temperature pseudo-Newtonian Keplerian accretion flow model for the millimeter and shorter wavelength emission from Sagittarius A*. A gene…

astro-ph2008★ 27 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…