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Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/74388

Type: Journal article
Title: 3 to 12 millimetre studies of dense gas towards the western rim of supernova remnant RX J1713.7-3946
Author: Maxted, Nigel Ivan
Rowell, Gavin Peter
Dawson, Bruce Robert
Burton, Michael G.
Nicholas, Brent Patrick
Fukui, Yasuo
Walsh, Andrew J.
Kawamura, Akiko
Horachi, Hirotaka
Sano, Hidetoshi
Citation: Monthly Notices of the Royal Astronomical Society, 2012; 422(3):2230-2245
Publisher: Blackwell Publishing Ltd
Issue Date: 2012
ISSN: 0035-8711
School/Discipline: School of Chemistry and Physics : Physics and Mathematical Physics
Statement of
Responsibility: 
Nigel I. Maxted, Gavin P. Rowell, Bruce R. Dawson, Michael G. Burton, Brent P. Nicholas, Yasuo Fukui, Andrew J. Walsh, Akiko Kawamura, Hirotaka Horachi and Hidetoshi Sano
Abstract: 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 such as CS(J= 1–0, J= 2–1) and its isotopologue counterparts, NH3(1, 1) and (2, 2) inversion transitions and N2H+(J= 1–0) emission, confirming the presence of dense gas ≳104 cm−3 in the region. The mass estimates for Core C range from 40 (from CS) to 80 M⊙ (from NH3 and N2H+), an order of magnitude smaller than published mass estimates from CO(J= 1–0) observations. We also modelled the energy-dependent diffusion of cosmic ray protons accelerated by RX J1713.7−3946 into Core C, approximating the core with average density and magnetic field values. We find that for considerably suppressed diffusion coefficients (factors χ= 10−3 down to 10−5 the Galactic average), low-energy cosmic rays can be prevented from entering the inner core region. Such an effect could lead to characteristic spectral behaviour in the GeV to TeV gamma-ray and multi-keV X-ray fluxes across the core. These features may be measurable with future gamma-ray and multi-keV telescopes offering arcminute or better angular resolution, and can be a novel way to understand the level of cosmic ray acceleration in RX J1713.7−3946 and the transport properties of cosmic rays in the dense molecular cores.
Keywords: diffusion – molecular data – supernovae; individual; RXJ1713.7−3946 – ISM; clouds – cosmic rays – gamma-rays; ISM
Rights: ©2012 The Authors. Monthly Notices of the Royal Astronomical Society C ©2012 RAS
RMID: 0020119307
DOI: 10.1111/j.1365-2966.2012.20766.x
Appears in Collections:Physics Publications
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