C1 non-LTE spectral line formation in late-type stars

Fabbian, Damian; Asplund, Martin; Carlsson, M.; Kisselman, D

Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

C1 non-LTE spectral line formation in late-type stars

Date

2005

Authors

Fabbian, Damian

Asplund, Martin

Carlsson, M.

Kisselman, D

Publisher

Cambridge University Press

Abstract

We present non-Local Thermodynamic Equilibrium (non-LTE) calculations for neutral carbon spectral line formation, carried out for a grid of model atmospheres covering the range of late-type stars. The results of our detailed calculations suggest that the