Internal motions in H II regions

Details Internal motions in H II regions Internal motions in H II regions

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98.1002o&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, Oct. 1986, p. 1002-1004.

Astronomy and Astrophysics

Astronomy

1

Gas Dynamics, H Ii Regions, Turbulence, Nebulae, Stellar Winds

Scientific paper

The internal motions in H II regions are in two separate but related components, ordered motion originating from differences in pressure and from impulse due to forces such as the stellar winds, and random motion originating from the turbulent flow of the gas. Ordered motion now seems to be reasonably well understood to the first order, while recent observational material on turbulence indicates a pattern of behavior only similar to the expectations of turbulence theory, with poor agreement in many major details.

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