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Components of the Local Interstellar Medium

Published online by Cambridge University Press:  13 May 2016

J. L. Linsky ,
S. Redfield  and
B. Wood
J. L. Linsky
Affiliation:
JILA, University of Colorado, Boulder, CO 80309-0440 USA
S. Redfield
Affiliation:
JILA, University of Colorado, Boulder, CO 80309-0440 USA
B. Wood
Affiliation:
JILA, University of Colorado, Boulder, CO 80309-0440 USA

Abstract

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HST, EUVE, and Ca II spectra are providing critical velocity and column density data needed to identify individual stuctures (clouds) of warm gas in the local ISM. The Sun is located very close to the edge of and will soon leave the Local Interstellar Cloud (LIC). We will summarize the properties of the LIC and other nearby warm clouds.

Type
Session VII: Energetic Particles and the Local Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 595 - 598
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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