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Morphological and spectral studies of the shell-type supernova remnants RX J1713.7-3946 and RX J0852.0-4622 with H.E.S.S.
- Source :
- Multi-Messenger Approach to High-Energy Gamma-Ray Sources; 2007, p379-384, 6p
- Publication Year :
- 2007
-
Abstract
- In 2004 and 2005, the shell-type supernova remnants RX J1713.7-3946 and RX J0852.0-4622 were observed and detected with the complete H.E.S.S. array, a system of four Imaging Cherenkov Telescopes located in Namibia and dedicated to the observations of γ-rays above 100 GeV. The energy spectra of these two sources have been measured over a wide energy range and revealed an integral flux above 1 TeV similar to that of the Crab Nebula. Their morphologies were resolved with high accuracy with H.E.S.S. and exhibit a striking correlation with the X-ray images, thereby pioneering a technique of unambiguously identifying spatially extended γ-ray sources. The results of the observations will be presented. Similarities and differences between these two sources will be pointed out as well as possible implications. [ABSTRACT FROM AUTHOR]
- Subjects :
- NEBULAE
ASTRONOMY
ASTRONOMICAL instruments
SPECTRUM analysis
CRAB Nebula
Subjects
Details
- Language :
- English
- ISBNs :
- 9781402061172
- Database :
- Complementary Index
- Journal :
- Multi-Messenger Approach to High-Energy Gamma-Ray Sources
- Publication Type :
- Book
- Accession number :
- 33098067
- Full Text :
- https://doi.org/10.1007/978-1-4020-6118-9_58