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.
The physical properties of the “local fluff”
Advances in Space Research ; 6 , 1 ; 345-351
01.01.1986
7 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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