Coronal Physics and the Chandra Emission Line Project

Abstract

With the launch of the Chandra X-ray Observatory, high resolution X-ray spectroscopy of cosmic sources has begun. Early, deep observations of three stellar coronal sources—Capella, Procyon, and HR 1099—are providing not only invaluable calibration data, but also benchmarks for plasma spectral models. These models are needed to interpret data from stellar… (More)

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Cite this paper

@inproceedings{BrickhouseCoronalPA, title={Coronal Physics and the Chandra Emission Line Project}, author={Nancy S. Brickhouse} }