The clumping factor in H II regions

Details The clumping factor in H II regions The clumping factor in H II regions

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61..715l&link_type=abstract

Astronomy and Astrophysics, vol. 61, no. 5, Dec. 1977, p. 715-717.

Astronomy and Astrophysics

Astrophysics

1

Galaxies, Gas Density, H Ii Regions, Hydrogen Ions, Interstellar Space, Clumps, Cosmic Gases, Electron Density (Concentration), Filling, Particle Emission, Planetary Nebulae

Scientific paper

A statistical method is developed for computing the average clumping factor inside the H II regions of the galaxy M33 by comparing on the same line of sight the integrated emission measure and the integrated neutral hydrogen measure. Using 136 H II regions, this method leads to an upper limit of 2.5 for the clumping factor or a filling factor of more than 40 percent.

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