Monochromatic radii: a tool of Mira diagnostics

Details Monochromatic radii: a tool of Mira diagnostics Monochromatic radii: a tool of Mira diagnostics

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..111s&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Monochromatic Radii, Mira Variables, Mira Atmospheres

Scientific paper

The shape and the wavelength-dependence of the brightness distribution on the stellar disk at different variability phases and cycles provides a powerful tool of diagnostics of the physical and geometric structure of the atmosphere of M-type Mira variables. In particular, the stratification of outer atmospheric layers may strongly affect brightness distributions and derived monochromatic diameters in a characteristic way.

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