Hydrodynamical models of the Orion-KL Nebula

Details Hydrodynamical models of the Orion-KL Nebula Hydrodynamical models of the Orion-KL Nebula

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..115o&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Statistics

Computation

Hydrodynamics, Molecular Clouds, Orion Nebula, Protostars, Stellar Winds, Computational Astrophysics, Density Distribution, Hydrogen, Polar Coordinates, Radial Velocity, Temperature Distribution

Scientific paper

The interaction between an isotropic protostellar wind and an ambient
molecular cloud is investigated by two-dimensional hydrodynamic
computations. The wind-cloud interaction model is promising for
explanation of the observed properties of the Orion-KL Nebula.

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