Chandra Observation of PWN G16.73+0.08 in SNR G16.7+0.7
碩士 === 國立清華大學 === 天文研究所 === 107 === Pulsar wind nebulae (PWNe) inside supernova remnants (SNRs) can have very different morphology when they interact with surrounding material. Detailed observations can help us to understand those manifestations of SNR and PWN. With the models of PWN/SNR evolution,...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2019
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| Online Access: | http://ndltd.ncl.edu.tw/handle/bkr76e |