An Observational Upper Limit on the Interstellar Number Density of Asteroids and Comets
We derived 90% confidence limits (CLs) on the interstellar number density (rho(CL)(IS)) of interstellar objects (ISOs; comets and asteroids) as a function of the slope of their size-frequency distribution (SFD) and limiting absolute magnitude. To account for gravitational focusing, we first generate...
Main Authors: | , , , , , , |
---|---|
Other Authors: | |
Language: | en |
Published: |
IOP PUBLISHING LTD
2017
|
Subjects: | |
Online Access: | http://hdl.handle.net/10150/623256 http://arizona.openrepository.com/arizona/handle/10150/623256 |