DYNAMICS OF IONIZED REGIONSReportar como inadecuado

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Abstract : Early type stars embedded in ionized regions may possess mechanical as well as radiative energy outputs. The mechanical energy output takes the form of a high velocity stellar wind. These winds may greatly affect the structure of the surrounding nebular material. A dis- cussion of possible dynamical and morphological effects is given.

Autor: J. Dyson

Fuente: https://hal.archives-ouvertes.fr/


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