Local Interstellar Matter: The view from Paris
天体物理学
2007-05-23 v1
摘要
Observations of interstellar gas and dust towards nearby stars and within the solar system show that the Sun is embedded in a warm diffuse partially-ionized cloud. This cloud is the leading edge of a flow of interstellar matter (ISM) through our Galactic neighborhood. Interstellar matter sets the boundary conditions of the heliosphere and astrospheres of extra-solar planetary systems. Moreover, the interplanetary regions in these systems are sensitive to inflowing ISM.
引用
@article{arxiv.astro-ph/0109300,
title = {Local Interstellar Matter: The view from Paris},
author = {Priscilla C. Frisch},
journal= {arXiv preprint arXiv:astro-ph/0109300},
year = {2007}
}
备注
XVIIth IAP Conference on Gaseous Matter in Galaxies and Intergalactic Space