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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    Titel :

    The physical properties of the “local fluff”


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    01.01.1986


    Format / Umfang :

    7 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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