A PHYSICAL MODEL FOR THE IRAS ZODIACAL DUST BANDS

被引：12
|
作者：
JONES, MH [1 ]
ROWANROBINSON, M [1 ]
机构：
[1] QUEEN MARY & WESTFIELD COLL, SCH MATH SCI, ASTRON UNIT, LONDON E1 4NS, ENGLAND
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 264卷 / 01期
关键词：
INTERPLANETARY MEDIUM; SOLAR SYSTEM; GENERAL; INFRARED;
D O I：
10.1093/mnras/264.1.237
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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 IRAS. In addition to the narrow asteroidal bands that have been previously reported, we find a broad double-band component with peak intensities at beta almost-equal-to +/- 9-degrees, which shows significant emission at latitudes \beta\ approximately 20-degrees. The physical significance of this feature within the Solar system and its relationship to the zodiacal cloud are discussed.
引用
收藏
页码：237 / 247
页数：11
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