Bibcode
Relaño, M.; Beckman, J. E.; Rozas, M.
Referencia bibliográfica
Chinese Journal of Astronomy and Astrophysics, Vol. 3, Supplement, p. 181-185
Fecha de publicación:
12
2003
Número de citas
0
Número de citas referidas
0
Descripción
We analyze the Hα emission line profiles of the HII region
populations in three disc spiral galaxies and find evidence of wing
features at 40-90 km/s from the central peak in a significant fraction
of regions. We explain the wing features as due to a shell expanding
inside the HII region, quantify the energy involved and present two
possible mechanisms to drive the expanding shell.