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The Transparency of Solar Coronal Active Regions
N. S. Brickhouse, J. T. Schmelz
Resonance scattering has often been invoked to explain the disagreement between the observed and predicted line ratios of Fe XVII 15.01 A to Fe XVII 15.26 A (the ``3C/3D'' ratio).…
A Hot Wind from the Classical T Tauri Stars: TW Hydrae and T Tauri
A. K. Dupree, N. S. Brickhouse, Graeme H. Smith +1
Spectroscopy of the infrared He I (10830A) line with KECK/NIRSPEC and IRTF/CSHELL, and of the ultraviolet C III (977A) and O VI (1032A) emission with FUSE reveals that the classica…
X-ray Light Curves and Accretion Disk Structure of EX Hydrae
R. Hoogerwerf, N. S. Brickhouse, C. W. Mauche
We present X-ray light curves for the cataclysmic variable EX Hydrae obtained with the Chandra High Energy Transmission Grating Spectrometer and the Extreme Ultraviolet Explorer De…
An Assessment of the Fe XVIII and Fe XIX Line Ratios from the Chandra Grating Observations of Capella
P. Desai, N. S. Brickhouse, J. J. Drake +8
Observations of Fe XVIII and Fe XIX X-ray, EUV, and FUV line emission, formed at the peak of Capella's (alpha Aurigae) emission measure distribution and ubiquitous in spectra of ma…