Hostname: page-component-6766d58669-88psn Total loading time: 0 Render date: 2026-05-23T23:36:17.566Z Has data issue: false hasContentIssue false

Molecules at the Interface of an HVC and a High-z HI Filament

Published online by Cambridge University Press:  12 April 2016

U. Mebold
Affiliation:
Radioastronomisches Institut der Universität Bonn Auf dem Hügel 71, D 5300 Bonn 1, F.R.G.
U. Herbstmeier
Affiliation:
Radioastronomisches Institut der Universität Bonn Auf dem Hügel 71, D 5300 Bonn 1, F.R.G.
P.W.M. Kalberla
Affiliation:
Radioastronomisches Institut der Universität Bonn Auf dem Hügel 71, D 5300 Bonn 1, F.R.G.
I. Souvatzis
Affiliation:
Radioastronomisches Institut der Universität Bonn Auf dem Hügel 71, D 5300 Bonn 1, F.R.G.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the 'Save PDF' action button.

The Draco nebula, the faint reflection nebulosity LBN 406/412/415 (Lynds 1965) at 1≈91°, b≈38°, z≥500 pc (Goerigk and Mebold, 1986), contains delicate filaments at its low-1, low-b (SW) boundary (Goerigk et al. 1983, Mebold et al. 1985). The density in the boundary is characterized by the presence of molecules like CO and H2CO (Mebold et al. 1985) and NH3 (Mebold et al. 1987). Johnson (1986) found an excess of unidentified IRAS point sources in the area of the Draco nebula, a large fraction of which is located close to the SW boundary.

Information

Type
VI. Interstellar Matter at High Galactic Latitudes
Copyright
Copyright © Springer-Verlag 1989