Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/82846
Citations | ||
Scopus | Web of Science® | Altmetric |
---|---|---|
?
|
?
|
Type: | Conference paper |
Title: | Dense gas towards the RXJ1713.7-3946 supernova remnant |
Author: | Maxted, N. Rowell, G. Dawson, B. Burton, M. Fukui, Y. Walsh, A. Kawamura, A. Sano, H. Lazendic, J. |
Citation: | High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy, Heidelberg, Germany 9 – 13 July 2012 / F. A. Aharonian, W. Hofmann, F. M. Rieger (eds.): pp. 253-256 |
Publisher: | American Institute of Physics |
Issue Date: | 2012 |
Series/Report no.: | AIP Conference Proceedings |
ISBN: | 9780735411234 |
ISSN: | 0094-243X 1551-7616 |
Conference Name: | International Meeting on High Energy Gamma-Ray Astronomy (5th : 2012 : Heidelberg, Germany) |
Editor: | Aharonian, F.A. Hofmann, W. Rieger, F.M. |
Statement of Responsibility: | Nigel I. Maxted, Gavin P. Rowell, Bruce R. Dawson, Michael G. Burton, Yasuo Fukui, Andrew J. Walsh, Akiko Kawamura, Hidetoshi Sano and Jasmina Lazendic |
Abstract: | 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. © 2012 American Institute of Physics. |
Keywords: | Molecular clouds H2 clouds Interstellar masers Supernova remnants γ -ray sources Cosmic rays |
Rights: | © 2012 American Institute of Physics |
DOI: | 10.1063/1.4772245 |
Published version: | http://dx.doi.org/10.1063/1.4772245 |
Appears in Collections: | Aurora harvest IPAS publications |
Files in This Item:
There are no files associated with this item.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.