NDLI: Asteroidal Dust and the Zodiacal Emission

Content Provider	Scilit
Author	Reach, William T.
Copyright Year	1991
Description	The contribution to the brightness of the infrared background by asteroidal dust, distinguished both by lower color temperature and ‘band-pair’ morphology, is determined using IRAS observations. Dust band pairs are associated with at least 7 asteroid families and groups, but very little is detected from the remainder of the asteroid belt, indicating that asteroid families and groups are the source of asteroidal dust.
Related Links	https://www.cambridge.org/core/services/aop-cambridge-core/content/view/03984FDCB71EB2E6937507C66FCD5592/S025292110006680Xa.pdf/div-class-title-asteroidal-dust-and-the-zodiacal-emission-div.pdf
Ending Page	214
Page Count	4
Starting Page	211
ISSN	02529211
DOI	10.1017/s025292110006680x
Journal	International Astronomical Union Colloquium
Volume Number	126
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	1991-01-01
Access Restriction	Open
Subject Keyword	International Astronomical Union Colloquium Astronomy and Astrophysics Asteroid Families Band Pairs Determined Using Zodiacal Emission Iras Observations Lower Color Infrared Background Color Temperature Dust Band
Content Type	Text
Resource Type	Article

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