Volume Filling Factors of ISM Phases and Turbulent Structure

Details Volume Filling Factors of ISM Phases and Turbulent Structure Volume Filling Factors of ISM Phases and Turbulent Structure

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ptep.proc...61b&link_type=abstract

Plasma Turbulence and Energetic Particles in Astrophysics, Proceedings of the International Conference, Cracow (Poland), 5-10 Se

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

The volume filling factors in the Galactic disk of H II, H I, H2 and dust are studied. The filling factors of ionized and molecular clouds as a function of mean cloud density follow similar power laws, suggesting that the two phases have similar structure. The size distributions of the clouds of H II and H2 as well as their mass distributions also have similar slopes, and are in agreement with fractional Brownian motion structure.

Affiliated with

Also associated with

No associations

Rating

Volume Filling Factors of ISM Phases and Turbulent Structure 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 Volume Filling Factors of ISM Phases and Turbulent Structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Volume Filling Factors of ISM Phases and Turbulent Structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1584495