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![]() Robin Shelton ASSOCIATE PROFESSOR OF PHYSICS |
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Research Interests My research explores the interstellar medium, the gas between the stars in our galaxy. Some of this gas is heated to millions of degrees by the most explosive events in the galaxy, supernova explosions. In order to estimate how supernova remnant bubbles affect parts of our galaxy and in order to study particular microphysical processes, I perform computer simulations. When tests of the theoretical and computational predictions require additional astronomical observations, I use X-ray and ultraviolet telescopes (mounted on satellites) to observe individual supernova remnant bubbles and the general interstellar medium. Recent
Publications
R. J.
Chastain, R. W. R. Oegerle, Jenkins, E. B., Shelton, R.L., Bowen, D. V., Chayer, P.,
"A Survey of O VI Absorption in the Local Interstellar Medium", Astrophysical Journal, 622, 377 (2005) R. M. Williams, R. M., Chu, Y.-H., Dickel, J. R., Gruendl, R. A., Shelton, R.,
Points, S. D., Smith, R. C.,
"Remnants in the Magellanic Clouds. IV. X-Ray Emission from the Largest
Supernova Remnant in the Large Magellanic Cloud", Astrophysical Journal, 613, 948 (2004) R. L. Shelton, K. D. Kuntz, & R. Petre,"'Chandra' Observations and Models of the Mixed-Morphology Supernova Remnant W44: Global Trends", Astrophys. J. 611, 906 (2004). B.-G. Andersson, D. C. Knauth, S. L. Snowden, R. L. Shelton, & P. G. Wannier, "A Hot Envelope Around the Southern Coalsack: X-ray and Far-Ultraviolet Observations", Astrophys. J. 606, 341 (2004).
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