PM. 04 Stars, Atmospheres, and Shells: Potential for High-Resolution Imaging

Details PM. 04 Stars, Atmospheres, and Shells: Potential for High-Resolution Imaging PM. 04 Stars, Atmospheres, and Shells: Potential for High-Resolution Imaging

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baas...16..797d&link_type=abstract

Bulletin of the American Astronomical Society, Vol. 16, p.797

Physics

Scientific paper

Substantial progress in stellar physics can result from one- or two-dimensional imaging at a spatial resolution of 10-3 to 10-5arc sec. The direct measurement of stellar diameters, surface and atmospheric features, and extended shells can significantly advance the knowledge of stellar structure, activity, and evolution. A dwarf star - the sun - and a supergiant star - Alpha Orionis - are used to illustrate the possibilities of measurements with high spatial resolution. In addition, magnetically sensitive lines can trace the distribution of activity across a stellar surface.

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