Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra
We have modelled the stellar and nebular continua and emission-line intensity ratios of massive stellar populations in the Antennae galaxy using high resolution and self-consistent libraries of model H II regions around central clusters of ageing stars. The model libraries are constructed using the stellar population synthesis code, STARBURST99
Gunawardhana, M. L. P. et al.
Fecha de publicación:
8
2020