Adelaide Research & Scholarship
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https://hdl.handle.net/2440/39765
| Type: | Conference paper |
| Title: | H.E.S.S. Observations of Shell Type SNR |
| Author: | Rowell, G. Berge, D. Hinton, J. |
| Citation: | 29th International Cosmic Ray Conference, August 3-10, 2005, Pune, India: [volume 4] / pp. 101-106 |
| Publisher: | Tata Institute of Fundamental Research |
| Issue Date: | 2005 |
| Conference Name: | International Cosmic Ray Conference (29th : 2005 : Pune, India) |
| Statement of Responsibility: | G.P. Rowell, D. Berge, J.A. Hinton, for the H.E.S.S. Collaboration |
| Abstract: | Over the past few years, H.E.S.S. has observed a number of shell-type supernova remnants (SNRs) in order to determine if they are capable of multi-TeV particle acceleration. Apart from RX J1713.7-3946 and RX J0852.0-4622 (Vela Junior) discussed separately at this conference, other candidates such as W28, SN 1987A, IC-443, Monoceros Loop/Rosette Nebula and SN 1006 are among several highly-ranked targets, based on previous TeV results and/or multi-wavelength information. We briefly outline the motivation for these H.E.S.S. observations and summarise details of several candidates. |
| Appears in Collections: | Aurora harvest Physics publications |
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