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Star counts and ammonia observations in the central Taurus region

  • H. Ungerechts
  • G. Winnewisser
  • M. Gaida
Part II: Compared Internal Structure of Nearby Molecular Clouds
Part of the Lecture Notes in Physics book series (LNP, volume 237)

Abstract

In summary, the cold cloud cores in Taurus have temperatures close to 10K,densities of about 104.5 cm-3, linewidths0.2-0.35km/s, and linear sizes 0.05-O.lpc. These paramters imply that they are close to thermal - gravitational equilibrium.

Keywords

Brightness Temperature Cloud Core Inversion Transition Cold Core Visual Extinction 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag 1985

Authors and Affiliations

  • H. Ungerechts
    • 1
  • G. Winnewisser
    • 1
  • M. Gaida
    • 1
  1. 1.I. Physikalisches Institut der Universität zu KölnKöln 41Germany

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