Abstract
I discuss the general problem of mapping the spatial structure in the atmospheres of active, late-type stars. There are several major differences between the problems of imaging photospheres and of imaging chromospheres. Because of these differences, chromospheric spectral imaging must be based on a direct decomposition of the observed emission line profiles.
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© 1990 Kluwer Academic Publishers
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Neff, J.E. (1990). Spatial Resolution of Stellar Atmospheres within Active Close Binaries. In: İbanoğlu, C. (eds) Active Close Binaries. NATO ASI Series, vol 319. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0679-2_56
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DOI: https://doi.org/10.1007/978-94-009-0679-2_56
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