Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-05T03:25:59.817Z Has data issue: false hasContentIssue false
  • English
  • Français

Oh Observations Near the Reflection Nebulae Ngc 2068 and Ngc 2071

Published online by Cambridge University Press:  14 August 2015

L. E. B. Johansson ,
B. Höglund ,
A. Winnberg ,
Nguyen-Q-Rieu  and
W. M. Goss
L. E. B. Johansson
Affiliation:
Onsala Space Observatory, Onsala, Sweden
B. Höglund
Affiliation:
Onsala Space Observatory, Onsala, Sweden
A. Winnberg
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.
Nguyen-Q-Rieu
Affiliation:
Observatoire de Meudon, Meudon, France
W. M. Goss
Affiliation:
Kapteyn Astronomical Laboratory, Groningen, The Netherlands

Abstract

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.

Narrow OH emission lines at 1667 MHz, apparently from a Class I source, have been observed near the reflection nebula NGC 2071. The region contains many T Tauri stars. OH emission corresponding to the dust cloud north and east of NGC 2024 is also seen. At 1720 MHz the dust cloud component appears in absorption; presumably the isotropic 2.7 K cosmic background is being absorbed.

Type
Part 2: Galactic H ii Regions
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 301 - 302
Copyright
Copyright © Reidel 1974