Dense gas towards the RXJ1713.7-3946 supernova remnant

Nigel I. Maxted, Gavin P. Rowell, Bruce R. Dawson, Michael G. Burton, Yasuo Fukui, Andrew J. Walsh, Akiko Kawamura, Hidetoshi Sano, Jasmina Lazendic

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademicpeer-review

1 Citation (Scopus)


A summary of results from a 7 mm-wavelength survey towards the young X-ray and γ-ray-bright supernova remnant, RXJ1713.7-3946 (SNR G347.3-0.5) is presented. Using the Mopra telescope, the high critical density tracer CS(1-0) was targeted, complementing previous Nanten2 molecular gas studies of CO transitions. In hadronic γ-ray emission scenarios (p-p interactions), the mass of cosmic ray target material available is an important factor, so we estimate the mass of dense gas towards RX J1713.7-3946. Also of interest was the shock-tracing molecule, SiO. Although there was no evidence of SiO emission physically excited by the RXJ1713.7-3946 shock, a chance-discovery of vibrationallyexcited SiO(1-0) emission is likely to be a maser that is associated with an evolved star.

Original languageEnglish
Title of host publicationHigh Energy Gamma-Ray Astronomy - 5th International Meeting on High Energy Gamma-Ray Astronomy
Number of pages4
Publication statusPublished - 2012
Externally publishedYes
Event5th International Meeting on High Energy Gamma-Ray Astronomy - Heidelberg, Germany
Duration: 9 Jul 201213 Jul 2012

Publication series

NameAIP Conference Proceedings
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616


Conference5th International Meeting on High Energy Gamma-Ray Astronomy


  • γ-ray sources
  • Cosmic rays
  • Interstellar masers
  • Molecular clouds H2 clouds
  • Supernova remnants


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