The Magnetic Field in Highly Dense Molecular Clouds

The Magnetic Field in Highly Dense Molecular Clouds

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 com...

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Veröffentlicht in:Symposium - International Astronomical Union 1990, Vol.140, p.268-268
1. Verfasser: El-Nawawy, M.S.
Format: Artikel
Sprache:eng
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Zusammenfassung: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.
ISSN:0074-1809
DOI:10.1017/S0074180900190199