The temperature of interstellar porous grains

Details The temperature of interstellar porous grains The temperature of interstellar porous grains

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..67..105b&link_type=abstract

Astrophysics and Space Science, vol. 67, no. 1, Jan. 1980, p. 105-110.

Astronomy and Astrophysics

Astrophysics

7

Granular Materials, Interstellar Matter, Porous Materials, Stellar Temperature, Graphite, Homogeneity, Lunar Rocks, Optical Properties, Silicates, Thermodynamic Equilibrium

Scientific paper

Free-space equilibrium temperatures for porous interstellar grains are computed for different dust sizes and are compared to those expected for homogeneous normal grains for two material candidates: graphite and a lunar silicate. Relevant differences are found with the former, but are essentially negligible with the latter. The results are discussed in terms of the different optical properties produced by the porosity of the grains. The possible astrophysical implications of these findings are also mentioned.

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