Tracing AGB Mass Loss by (Synthetic) High-Resolution IR Spectroscopy

Details Tracing AGB Mass Loss by (Synthetic) High-Resolution IR Spectroscopy Tracing AGB Mass Loss by (Synthetic) High-Resolution IR Spectroscopy

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..325n&link_type=abstract

Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes. ASP Conference Series, Vol. 378, proceedings of the co

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on recent advances in line profile modelling of different
near-infrared (NIR) molecular absorption features based on dynamic model
atmospheres for pulsating and mass-losing AGB stars (Mira variables).

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