Formation, Evolution and Disruption of Giant HII regions.
The distribution of velocity dispersion versus intensity, corresponding to the emission of the ionized gas over a giant HII region is explained within the framework of the cometary stirring model. The development of shells and loops generated by massive stars, which finally cause the cloud disruption, can also be followed with this representation.
Muñoz-Tuñon, C. et al.
Advertised on:
0
1996