Volume Filling Factors of the DIG in M 31

Details Volume Filling Factors of the DIG in M 31 Volume Filling Factors of the DIG in M 31

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.289..207b&link_type=abstract

Astrophysics and Space Science, v. 289, Issue 3, p. 207-210 (2004).

Astronomy and Astrophysics

Astrophysics

1

Dig, Filling Factor, Hii: Diffuse, Ism, M 31

Scientific paper

The volume filling factor f v of the diffuse ionized gas in the bright emission ring of M 31 is derived from radio continuumobservations. The dependence of f v on the local mean electron density n e is a power law, f v(n e) = a n e -bwith a = 0.011± 0.003 and b = -1.2± 0.3, where n e is in cm-3. The same power law was recently found for the DIG in the solar neighbourhood from pulsar data.

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