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3 to 12 millimetre studies of dense gas towards the western rim of supernova remnant RX J1713.7-3946
12 millimetre dense gas the western rim supernova remnant RX J1713.7-3946
2012/2/23
The young X-ray and gamma-ray-bright supernova remnant RXJ1713.7-3946 (SNR G347.3-0.5) is believed to be associated with molecular cores that lie within regions of the most intense TeV emission. Using...
A Detailed Study of the Molecular and Atomic Gas Toward the γ-ray SNR RX J1713.7-3946: Spatial TeV γ-ray and ISM Gas Correspondence
McClure-Griffi ths G. Rowel T. Inoue S. Inutsuka A. Kawamura
2011/9/27
RX J1713.7-3946 is the most remarkable TeV {\gamma}-ray SNR which emits {\gamma}-rays in the highest energy range 10-100 TeV. We made a combined analysis of CO and HI in the SNR and derived the total ...
Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946
Modeling the Multi-Wavelength Emission Shell-Type Supernova Remnant
2010/11/9
Emission mechanisms of the shell-type supernova remnant (SNR) RX J1713.7-3946 are studied with multi-wavelength observational data from radio, X-ray,GeV γ-ray to TeV γ-ray band. A Markov Chain Monte C...