Are molecular clouds formed by impact of High-Velocity Clouds?

Details Are molecular clouds formed by impact of High-Velocity Clouds? Are molecular clouds formed by impact of High-Velocity Clouds?

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..195l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 195-197

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Hydrodynamics, Interstellar Chemistry, Molecular Clouds, Molecular Gases, Spatial Distribution, Star Clusters, Star Formation, Stars, Computerized Simulation, Concentration (Composition), Morphology, Normal Density Functions, Orion Constellation, Velocity

Scientific paper

We simulated collisions of High Velocity Clouds (HVCs) with the galactic disk with a simple hydrodynamical code. Main aspects of the morphology of nearby (d less than 500 pc) cloud complexes, like the rho Oph, Orion and Taurus-Auriga-Perseus complexes, are reproduced. These aspects include total mass, distance from the galactic plane, orientation of elongated gas structures with respect to the plane, and relative position of clusters of O-B stars with respect to the main concentrations of molecular gas. The space distribution of stars of different ages, usually explained in terms of sequential star formation, is interpreted in a new way in our model.

Affiliated with

Also associated with

No associations

Rating

Are molecular clouds formed by impact of High-Velocity Clouds? 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 Are molecular clouds formed by impact of High-Velocity Clouds?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Are molecular clouds formed by impact of High-Velocity Clouds? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1252776