Millimetre Wave Emission by Interstellar Dust

Details Millimetre Wave Emission by Interstellar Dust Millimetre Wave Emission by Interstellar Dust

Sep 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.223.1143l&link_type=abstract

Nature, Volume 223, Issue 5211, pp. 1143-1144 (1969).

Physics

2

Scientific paper

IF the interstellar grains consist of material resembling a semiconductor with a d.c. conductivity σ in the range 0.01 to 10 Ω-1 cm-1, then there may be large optical depths for millimetre and submillimetre waves due to grains. Thus dense clouds or condensations within them may be significant blackbody radiators at these wavelengths because of the grains. Because the grains may have amorphous but not glassy structure, or contain impurities and lattice defects even if the structure should be well ordered, such conductivities for the grains are highly probable1,2.

Affiliated with

Also associated with

No associations

Rating

Millimetre Wave Emission by Interstellar Dust 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 Millimetre Wave Emission by Interstellar Dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Millimetre Wave Emission by Interstellar Dust will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1426596