activity
19962009
most citedExploring cloudy gas accretion as a source of interstellar turbulence in the outskirts of disks

22 citations · 26 across the 4 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008

The Role of the Random Magnetic Fields in the ISM: HVCs Numerical Simulations

A. Santillan, J. Kim, F. J. Sanchez-Salcedo +2

We know that the galactic magnetic field possesses a random component in addition to the mean uniform component, with comparable strength of the two components. This random compone…

astro-ph20084 cited

On the origin of the neutral hydrogen supershells: the ionized progenitors and the limitations of the multiple supernovae hypothesis

Sergiy Silich, Federico Elias, José Franco

Here we address the question whether the ionized shells associated with giant HII regions can be progenitors of the larger HI shell-like objects found in the Milky Way and other sp…

astro-ph200722 cited

Exploring cloudy gas accretion as a source of interstellar turbulence in the outskirts of disks

A. Santillan, F. J. Sanchez-Salcedo, J. Franco

High--resolution 2D--MHD numerical simulations have been carried out to investigate the effects of continuing infall of clumpy gas in extended HI galactic disks. Given a certain ac…

astro-ph2004

Magnetic-Driven Winds from Post-AGB Stars: Solutions for High Speed Winds and Extreme Collimation

Guillermo Garcia-Segura, Jose Alberto Lopez, Jose Franco

This paper explores the effects of post-AGB winds driven solely by magnetic pressure from the stellar surface. It is found that winds can reach high speeds under this assumption, a…

astro-ph2001

Ultracompact HII Regions

Stan Kurtz, Jose Franco

We review some recent observational results on the properties of ultracompact HII regions, in particular the presence of extended continuum emission surrounding ultracompact source…

astro-ph2001

Late AGB Magnetic Cycles: MHD Solutions for the HST PN Rings

Guillermo Garcia-Segura, Jose Alberto Lopez, Jose Franco

The Hubble Space Telescope has revealed the existence of multiple, regularly spaced, and faint concentric shells around some planetary nebulae. Here we present 2(1/2)D magnetohydro…