Interaction of High Velocity Clouds with Magnetized Disks: Three-Dimensional Numerical Simulations

Details Interaction of High Velocity Clouds with Magnetized Disks: Three-Dimensional Numerical Simulations Interaction of High Velocity Clouds with Magnetized Disks: Three-Dimensional Numerical Simulations

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004jkas...37..233s&link_type=abstract

Journal of the Korean Astronomical Society, vol. 37, no. 4, pp. 233-235

Astronomy and Astrophysics

Astronomy

2

Ism: Clouds, Ism: Magnetic Fields, Ism, Mhd

Scientific paper

High-velocity clouds are flows of neutral hydrogen, located at high galactic latitudes, with large velocities (mid VLSR mid ≥ 100 km/s) that do not match a simple model of circular rotation for our Galaxy. Numerical simulations have been performed for the last 20 years to study the details of their evolution, and their possible interaction with the Galactic disk. Here we present a brief review of the models that have been already published, and describe newly performed three-dimensional magnetohydrodynamic simulations.

Affiliated with

Also associated with

No associations

Rating

Interaction of High Velocity Clouds with Magnetized Disks: Three-Dimensional Numerical Simulations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Interaction of High Velocity Clouds with Magnetized Disks: Three-Dimensional Numerical Simulations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interaction of High Velocity Clouds with Magnetized Disks: Three-Dimensional Numerical Simulations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1086150