3 to 12 millimetre studies of dense gas towards the western rim of supernova remnant RX J1713.7-3946

3 to 12 millimetre studies of dense gas towards the western rim of supernova remnant RX J1713.7-3946

The young X-ray and gamma-ray-bright supernova remnant RX J1713.7−3946 (SNR G347.3−0.5) is believed to be associated with molecular cores that lie within regions of the most intense TeV emission. Using the Mopra telescope, four of the densest cores were observed using high critical density tracers s...

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Bibliographic Details
Main Authors: Maxted, N., Rowell, G., Dawson, B., Burton, M., Nicholas, B., Fukui, Y., Walsh, Andrew, Kawamura, A., Horachi, H., Sano, H.
Format: Journal Article
Published: Oxford University Press 2012
Subjects:
diffusion
gamma-rays: ISM
ISM: clouds
supernovae: individual: RX J1713.7-3946
cosmic rays
molecular data
Online Access:http://hdl.handle.net/20.500.11937/18107

Internet

http://hdl.handle.net/20.500.11937/18107

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