In:
International Astronomical Union Colloquium, Cambridge University Press (CUP), Vol. 81 ( 1984), p. 243-247
Kurzfassung:
21-cm line observations with the Westerbork Synthesis Radio Telescope of a dust and molecular filament at the boundary of the Draco Nebula (l≈ 91°, b≈ 38°) reveal a jet-like neutral hydrogen feature funneling through an outlet in the low velocity shock front at the interface between the Draco Nebula and the surrounding gas. The jet-like feature is apparently connected with a high velocity filament at VLSR = -180 km s -1 . We suggest that the soft x-ray emission observed in the area is thermal bremsstrahlung produced by the deceleration of high velocity gas in galactic gas.
Materialart:
Online-Ressource
ISSN:
0252-9211
DOI:
10.1017/S0252921100098286
Sprache:
Englisch
Verlag:
Cambridge University Press (CUP)
Publikationsdatum:
1984
