Far-IR and submillimeter radiation from cometary and circumstellar dust

Details Far-IR and submillimeter radiation from cometary and circumstellar dust Far-IR and submillimeter radiation from cometary and circumstellar dust

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.315..113j&link_type=abstract

In ESA, Formation of Stars and Planets, and the Evolution of the Solar System p 113-120 (SEE N91-18922 10-90)

Astronomy and Astrophysics

Astronomy

2

Comet Tails, Cosmic Dust, Far Infrared Radiation, Interstellar Chemistry, Stellar Evolution, Submillimeter Waves, Accretion Disks, Chemical Analysis, Comet Nuclei, Infrared Astronomy, Stellar Mass Accretion

Scientific paper

An introduction to the emergent fields of cometary and stellar submillimeter astronomy is presented. Cometary and circumstellar dust grains may share a common origin in the accretion disks of pre-main sequence stars. Far IR and submillimeter radiation from these grains are used to infer basic characteristics of the dust. Long wavelength measurements of comets and circumstellar dust clouds are discussed. The problems inherent in their interpretation are reviewed.

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