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An X-Ray Study of the Supernova Remnant G290.1-0.8
Patrick Slane, Randall K. Smith, John P. Hughes +1
G290.1-0.8 (MSH 11-61A) is a supernova remnant (SNR) whose X-ray morphology is centrally bright. However, unlike the class of X-ray composite SNRs whose centers are dominated by no…
Collisional Plasma Models with APEC/APED: Emission Line Diagnostics of Hydrogen-like and Helium-like Ions
Randall K. Smith, Nancy S. Brickhouse, Duane A. Liedahl +1
New X-ray observatories (Chandra and XMM-Newton) are providing a wealth of high-resolution X-ray spectra in which hydrogen- and helium-like ions are usually strong features. We pre…
X-ray Halos and Large Grains in the Diffuse Interstellar Medium
Adolf N. Witt, Randall K. Smith, Eli Dwek
Recent observations with dust detectors on board the interplanetary spacecraft Ulysses and Galileo have recorded a substantial flux of large interstellar grains with radii between…