A Physical Model for the IRAS Zodiacal Dust Bands

Details A Physical Model for the IRAS Zodiacal Dust Bands A Physical Model for the IRAS Zodiacal Dust Bands

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.264..237j&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 264, NO. 1/SEP1, P. 237, 1993

Astronomy and Astrophysics

Astronomy

7

Interplanetary Medium - Solar System: General - Infrared: Solar System

Scientific paper

We present a model, based on justifiable physical assumptions, of the zodiacal cloud and asteroidal dust bands which gives a good representation of the thermal IR emission from interplanetary dust observed using IRA& In addition to the narrow asteroidal bands that have been previously reported, we find a broad double-band component with peak intensities at β ≍ ±9°, which shows significant emission at latitudes |β| ˜ 20°. The physical significance of this feature within the Solar system and its relationship to the zodiacal cloud are discussed.

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