An Infra-Red model of the zodiacal emission |
| |
| Authors: | J. Tigg G. Pearce |
| |
| Affiliation: | (1) Lincoln College Oxford University, Oxford, U.K.;(2) Astrophysics Department, Oxford University, Jesus College, Oxford, U.K.;(3) Rutherford Appleton Laboratory, Chilton, Oxfordshire, England, U.K. |
| |
| Abstract: | The Infra-Red Astronomical Satellite (IRAS) observations of the zodiacal dust emission are used to fit the dust grain composition and distribution in the ecliptical plane. We obtain a good fit to the data for a density distribution of black-body grains given by p = pr0.66/log(1.7r/R) for r < 0.87R and r < 3oR |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
