The volume filling factor of the infrared cirrus IS 0.2

Details The volume filling factor of the infrared cirrus IS 0.2 The volume filling factor of the infrared cirrus IS 0.2

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...338..147v&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 338, March 1, 1989, p. 147-151. Research supported by the Alan and Dorothy

Astronomy and Astrophysics

Astronomy

17

Cosmic Dust, Infrared Sources (Astronomy), Interstellar Radiation, Molecular Clouds, Stellar Luminosity, Brightness Distribution, Emission Spectra, Infrared Astronomy Satellite, Radiation Distribution, Stellar Envelopes

Scientific paper

The filling factor of the infrared cirrus in which luminous stars are
embedded is estimated. The stars are assumed to be randomly situated
with respect to the cirrus. A direct ratio of the number of stars with
associated cirrus emission to those which in principle could be detected
indicates that the cirrus filling factor is roughly 0.2.

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