Suzaku and Fermi observations of the supernova remnant G1.9 + 0.3
Abstract
We present results from the observation of the supernova remnant (SNR) G1.9 + 0.3, which is the youngest known SNR in the Milky Way, with the X-ray imaging spectrometer (XIS) on board Suzaku. We investigate the nature of the X-ray emission and compare our results with the previous X-ray studies. Additionally, we present the analysis results of the GeV gamma-ray data taken for about 6 years by the Large Area Telescope on board Fermi and discuss these results in the framework of existing gamma-ray emission scenarios.
- Publication:
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Advances in Space Research
- Pub Date:
- October 2015
- DOI:
- 10.1016/j.asr.2015.07.018
- Bibcode:
- 2015AdSpR..56.1793G
- Keywords:
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- ISM: supernova remnants;
- ISM: G1.9 + 0.3;
- X-rays: ISM;
- Gamma rays: ISM