On the Shock-induced Variability of Emission Lines in M-type Mira Variables II. FeII and [FeII] emission lines as a diagnostic tool
Our observations of cool, shock penetrated, expanding atmospheres of M-type Mira variables (Richter & Wood 2001) have suggested that the emission lines of Fe II and [Fe II] can serve as an excellent diagnostic tool to study the hydro- and thermodynamical
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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