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• W1569288947 abstract "Abstract I provide examples of how high-resolution x-ray spectra may be used to determine the temperature and emission measure distributions, electron densities, steady and transient flow velocities, and location of active regions in stellar coronae. For each type of measurement I estimate the minimum spectral resolution required to resolve the most useful spectral features. In general, high sensitivity is required to obtain sufficient signal-to-noise to exploit the high spectral resolution. Although difficult, each measurement should be achievable with the instrumentation proposed for AXAF." @default.
• W1569288947 created "2016-06-24" @default.
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• W1569288947 date "1990-01-01" @default.
• W1569288947 modified "2023-09-25" @default.
• W1569288947 title "Goals for the Application of High-Resolution X-ray Spectroscopy to the Diagnosis of Stellar Coronal Plasmas" @default.
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• W1569288947 doi "https://doi.org/10.1017/s0252921100012197" @default.
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