HIGHLIGHTS
- who: Elisa Prandini and Gabriele Ghisellini from the Department of Physics and Astronomy, University of Padova, Via Marzolo, Padova, PD, Italy have published the research work: The Blazar Sequence and Its Physical Understanding, in the Journal: Galaxies 2022, 10, 35. of /2022/
- what: For the X-ray-selected sample, the analysis showed a tendency for u03b3-ray loud sources to have a larger radio luminosity and steeper radio and X-ray spectral indices.
- future: It would be detected in the MeV range by future generations of MeV satellites such as the eASTROGAM AMEGO . . .
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