Local Interstellar Matter: The view from Paris

Astronomy and Astrophysics – Astrophysics

Scientific paper

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XVIIth IAP Conference on Gaseous Matter in Galaxies and Intergalactic Space

Scientific paper

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.

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