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The global impact of stellar winds and supernovae on the interstellar medium [PDF]
, 2015 The interstellar medium is an extremely heterogeneous mixture of gas and dust which fills the space between stars in galaxies. The life-cycle of stars is deeply connected with the presence of this medium. Massive stars form from very high density/low temperature gas and evolve for millions of years.
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Reduced Models of Magnetohydrodynamic Turbulence in the Interstellar Medium and the Solar Wind
1999Recent developments in the derivation of reduced models for weakly compressible magnetohydrodynamic (MHD) turbulence are discussed. A four-field system of equations has been derived from the compressible magnetohydrodynamic (MHD) equations to describe turbulence in the interstellar medium and the solar wind.
A. Bhattacharjee, C.S. Ng
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Interaction of the solar wind with the local interstellar medium: a theoretical perspective
Space Science Reviews, 1999The interaction of the solar wind with the local interstellar medium (LISM) is attracting renewed interest, thanks to the possibility that the Voyager spacecraft may, in the not too distant future, cross the heliospheric termination shock. This has spurred the development of increasingly sophisticated models which attempt to describe various aspects of
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Astrospheres, stellar winds, and the interstellar medium
2016Brian E. Wood, Jeffrey L. Linsky
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Supernovae and Stellar Wind in the Interstellar Medium
Astrophysics and Space Science, 1997openaire +1 more source
The interaction of the solar wind with the local interstellar medium
Advances in Space Research, 1989openaire +1 more source
On the interaction of the solar wind with the interstellar medium: Field aligned MHD flow
Journal of Geophysical Research, 2002Romana Ratkiewicz
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