In Situ Measurements of Interstellar Dust
Astrophysics
2009-10-30 v1
Abstract
We present the mass distribution of interstellar grains measured in situ by the Galileo and Ulysses spaceprobes as cumulative flux. The derived in situ mass distribution per logarithmic size interval is compared to the distribution determined by fitting extinction measurements. Large grains measured in situ contribute significantly to the overall mass of dust in the local interstellar cloud. The problem of a dust-to-gas mass ratio that contradicts cosmic abundances is discussed.
Cite
@article{arxiv.astro-ph/9711190,
title = {In Situ Measurements of Interstellar Dust},
author = {M. Landgraf and E. Gruen},
journal= {arXiv preprint arXiv:astro-ph/9711190},
year = {2009}
}
Comments
4 pages and two figures