What do we do when models don't fit? On model atmospheres and real stellar spectra

• Developments in the modelling of stellar atmospheres and results from the confrontation between calculated and observed fluxes and spectra are discussed. It is argued that, although impressive advances in the study of O-type, WR and cool star spectra have

Nyckelord

COOL DWARF STARS; INCLUDING SPHERICAL EXTENSION; RADIATION-DRIVEN WINDS; BALMER-LINE-PROFILES; IRON-GROUP ELEMENTS; HOT LUMINOUS STARS; SOLAR GRANULATION; CARBON STARS; O-STARS; VEGA

Publikations- och innehållstyp

vet (ämneskategori)

art (ämneskategori)