Paper Summary by Mr Nigel Maxteed
Interstellar gas towards ctb 37a and the tev gamma-ray source hess j1714-385
The density of high-energy particles towards the remains of an exploded star is estimated. Our findings are consistent with a time of approximately 10 000 years passing since the star exploded.
Authors: Maxted, N.I., Rowell, G.P., Dawson, B.R., Burton, M.G., Fukui, Y., Walsh, A., Kawamura, A., Horachi, H., Sano, H., Yoshiike, S. & Fukuda, T.
This work was done in collaboration with researchers from University of New South Wales, Curtin University and Nagoya University, Japan
Monthly Notices of the Royal Astronomical Society 434 (3), 2188-2201 (2013)