The ionizing radiation from massive stars and its impact on HII regions: results from modern model atmospheres
We present a detailed comparison of the ionizing spectral energy distributions (SEDs) predicted by four modern stellar atmosphere codes, TLUSTY, CMFGEN, WM-basic and FASTWIND. We consider three sets of stellar parameters representing a late O-type dwarf (O9.5V), a mid-O-type (O7V) dwarf and an early O-type dwarf (O5.5V). We explore two different
Simón-Díaz, S. et al.
Fecha de publicación:
9
2008