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Abstract

The area between 168° ≦ lI ≦ 180°, − 2° ≦ bI ≦ + 5°, containing the I Mon association, was investigated by a study of the 21-cm-line emission of HI. The profiles were taken at discrete points with a distance of 1° in longitude and latitude; the receiver bandwidth being 30 kcps, the resolving power of the receiver was 1.5° K for an average profile used in the reduction.

Copyright information

© Springer Fachmedien Wiesbaden 1964

Authors and Affiliations

  • Hans-Günter Girnstein
    • 1
  1. 1.Sternwarte der Universität BonnDeutschland

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