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| Autor principal: | |
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| Formato: | Preprint |
| Publicado: |
2024
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| Materias: | |
| Acceso en línea: | https://arxiv.org/abs/2411.08525 |
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- The jet may compress an interstellar medium and soft X-ray may be absorbed outside the jet by a compressed interstellar medium and thermal emission heated by a shock is expected inside the jet. I analyze X-ray image of surroundings of the jet of M87 by Chandra. There is an original work for image analysis. In this time, I select data for image by removal of pile up event completely. I confirm a dip in soft X-ray outside the jet between knot E and knot F with 260 ks archival data. I analyze X-ray energy spectra for knot E and knot F with 400 ks archival data by Chandra in order to search for thermal emission. However, X-ray energy spectra for knot E and knot F are well described with synchrtron emission.