Optical and Near-IR Spectra of O-rich Mira Variables: A comparison between models and observations
Pulsation models are crucial for the interpretation of spectrophotometric and interferometric observations of Mira variables. Comparing predicted and observed spectra is one way of establishing the validity of such models. In this paper, we focus on the models published between 1996 and 1998 by Bessell, Hofmann, Scholz and Wood. A few new model spectra are added, to improve available phase coverage. We compare the synthetic spectra with observed low resolution spectra of optically selected...[Show more]
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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