X-ray Spectral Evolution of High Energy Peaked Blazars
The synchrotron hump of the high energy peaked blazars generally lies in the 0.1–10 keV range and such sources show extreme flux and spectral variability in X-ray bands. Various spectral studies showed that the X-ray spectra of high energy peaked blazars are curved and better described by the log-pa...
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| Format: | Article |
| Language: | English |
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MDPI AG
2020-08-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/8/3/62 |