Abstract Observations of interstellar gas in front of stars near the Sun are briefly reviewed to obtain for the properties of the local fluff: n−0.1 cm −3, n e 0.003 cm−3, T−11, 500 °K, and B−3−5 μG. The velocity vector obtained from He° λ584 backscattered data (V, 1, b) = (−25 km s −1, 3°, +17°) appears to adequately describe the heliocentric upwind velocity vector for the local fluff.


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    Title :

    The physical properties of the “local fluff”


    Contributors:

    Published in:

    Publication date :

    1986-01-01


    Size :

    7 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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