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A Neutral Gas Jet in a Low Velocity Shock Front at the Boundary of the Draco Nebula
Published online by Cambridge University Press: 12 April 2016
Abstract
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.
- Type
- The LISM at Infrared and Millimeter Wavelengths
- Information
- International Astronomical Union Colloquium , Volume 81: Local Interstellar Medium , 1984 , pp. 243 - 247
- Copyright
- Copyright © NASA 1984
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