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The Magnetic Field in Highly Dense Molecular Clouds

Published online by Cambridge University Press:  19 July 2016

M.S. El-Nawawy
M.S. El-Nawawy*
Affiliation:
1 Department of Astronomy, Faculty of Science Cairo University, Cairo, Egypt 2 present adress: Silberberg str.39/1 6901 Mauer, FRG

Extract

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General forms of the B-ρ relation are investigated in both the isothermal and the non-isothermal regions. The magnetic flux dissipation either by ambipolar diffusion or by Ohmic dissipation has been restudied. The rates of heating due to the magnetic dissipation processes have been calculated in comparison with the rate of compressional heating.

Type
6. Magnetic Fields in Molecular Clouds, Dark Globules and in the Pre-Stellar and Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 268
Copyright
Copyright © Kluwer 1990