Dense Gas Towards the RX J1713.7–3946 Supernova Remnant

Dense Gas Towards the RX J1713.7–3946 Supernova Remnant

We present results from a Mopra 7 mm-wavelength survey that targeted the dense gas-tracing CS(1-0) transition towards the young γ-ray-bright supernova remnant, RX J1713.7–3946 (SNR G 347.3−0.5). In a hadronic γ-ray emission scenario, where cosmic ray (CR) protons interact with gas to produce the obs...

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Bibliographic Details
Main Authors: Maxted, N., Rowell, G., Dawson, B., Burton, M., Fukui, Y., Lazendic, J., Kawamura, A., Horachi, H., Sano, H., Walsh, Andrew, Yoshiike, S., Fukuda, T.
Format: Journal Article
Published: CSIRO 2013
Subjects:
gamma rays: ISM
supernovae: individual: RX J1713.7–3946
ISM: clouds
molecular data
cosmic rays
Online Access:http://hdl.handle.net/20.500.11937/38909

Internet

http://hdl.handle.net/20.500.11937/38909

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