Quantifying the ionising flux escaping from the ultra-luminous HII regions in four spiral galaxies
There are two principal problems in explaining, in terms of the emission from OB stars, the ionisation of the gas which emits the diffuse H-alpha in spiral galaxies. One is the long pathlengths which the ionising photons need to traverse to reach their objectives, the other is whether sufficient photons can escape from within the HII regions which
Rozas, M. et al.
Fecha de publicación:
4
1998