Structure of Molecular Clouds

Details Structure of Molecular Clouds Structure of Molecular Clouds

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.292...89f&link_type=abstract

Astrophysics and Space Science, v. 292, Issue 1, p. 89-101 (2004).

Astronomy and Astrophysics

Astrophysics

18

Molecular Clouds, Turbulence, Fractals, Intermittency, Magnetic Fields

Scientific paper

This review, far from exhaustive, focuses on the specific properties of molecular clouds in their least condensed phase. Emphasis is placed on their connection with the diffuse medium, their multi-fractal characteristics and the diversity of their small-scale structure, where cold and dense gas may coexist with dilute and warm gas. Stuctures of essentially pure velocity origin are uncovered and seen as a possible signature of the intermittency of turbulence dissipation.

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