The spectral dependence of dust emissivity at millimeter wavelengths

Details The spectral dependence of dust emissivity at millimeter wavelengths The spectral dependence of dust emissivity at millimeter wavelengths

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...252..589s&link_type=abstract

Astrophysical Journal, Part 1, vol. 252, Jan. 15, 1982, p. 589-593.

Astronomy and Astrophysics

Astronomy

52

Brightness Temperature, Cosmic Dust, Interstellar Matter, Millimeter Waves, Molecular Clouds, Radio Sources (Astronomy), Spectral Emission, Temperature Gradients

Scientific paper

Millimeter wavelength (frequency less than or equal to 300 GHz) observations of the three objects NGC 2264, S 140, and NGC 6334N are analyzed and the power-law spectral dependence of dust emissivity derived. The spectral index is found to be steeper than quadratic, and it is concluded that silicate core grains with thin ice mantles are a likely grain material.

Affiliated with

Also associated with

No associations

Rating

The spectral dependence of dust emissivity at millimeter wavelengths does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The spectral dependence of dust emissivity at millimeter wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectral dependence of dust emissivity at millimeter wavelengths will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1455706