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The Intermediate Velocity Cloud IVC86+38.5-45, Related to High Velocity Clouds?

Published online by Cambridge University Press:  12 April 2016

U. Herbstmeier
U. Herbstmeier*
Affiliation:
Radioastronomisches Institut der Universität, Bonn

Extract

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Examining the high velocity cloud complex C and its possible interaction with gas of the galactic disk we became aware of a dust cloud located at galactic longitude l = 86° and latitude b = 38°.5 seen in the l00µm image of the IRAS. This cloud consists of a cucumber shaped core surounded by a horseshoe shaped halo opening towards larger galactic coordinates. At very low 100µm intensities dust lanes starting at the core or the ends of the horseshoe can be traced for about 5° towards high galactic latitude and longitude.

Type
VI. Interstellar Matter at High Galactic Latitudes
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 458
Copyright
Copyright © Springer-Verlag 1989