Structure of molecular clouds. III - Effects of MHD waves in collapsing fragments

Details Structure of molecular clouds. III - Effects of MHD waves in collapsing fragments Structure of molecular clouds. III - Effects of MHD waves in collapsing fragments

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....90..134m&link_type=abstract

Astronomy and Astrophysics, vol. 90, no. 1-2, Oct. 1980, p. 134-139. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

8

Magnetohydrodynamic Waves, Molecular Clouds, Protostars, Radio Emission, Spectral Signatures, Carbon Monoxide, Emission Spectra, Line Shape, Line Spectra, Magnetic Field Configurations, Stellar Evolution, Stellar Structure, Wave Propagation

Scientific paper

The signature of early protostars in CO line emission was calculated, taking into account the possibility that MHD waves may be generated in the differentially rotating core. The result obtained was that the CO line shape of unresolved protostars is broadened, corresponding to supersonic but sub-Alfvenic turbulent velocities, and that it has extended low intensity wings.

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