Local Interstellar Matter: The view from Paris

Simple item page
dc.creatorFrisch, Priscilla C.
dc.date2001-09-18
dc.date.accessioned2026-07-07T02:00:02Z
dc.date.available2026-07-07T02:00:02Z
dc.descriptionObservations 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.
dc.descriptionXVIIth IAP Conference on Gaseous Matter in Galaxies and Intergalactic Space
dc.identifierhttps://arxiv.org/abs/astro-ph/0109300
dc.identifierhttp://arxiv.org/abs/astro-ph/0109300
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3343
dc.subjectAstrophysics
dc.titleLocal Interstellar Matter: The view from Paris
dc.typetext

Files

Collections

arXiv