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pro vyhledávání: '"Palit, B."'
Autor:
Palit, B., Rozanska, A., Petrucci, P. O., Gronkiewicz, D., Barnier, S., Bianchi, S., Ballantyne, D. R., Gianolli, V. E., Middei, R., Belmont, R., Ursini, F.
In the X-ray spectra of AGNs, a noticeable excess of soft X-rays is typically detected beyond the extrapolation of the power-law trend observed between 2-10 keV. In the scenario of warm Comptonization, observations propose a warm corona temperature r
Externí odkaz:
http://arxiv.org/abs/2406.14378
Autor:
Ballantyne, D. R., Sudhakar, V., Fairfax, D., Bianchi, S., Czerny, B., De Rosa, A., De Marco, B., Middei, R., Palit, B., Petrucci, P. -O., Rozanska, A., Ursini, F.
The soft excess in active galactic nuclei (AGNs) may arise through a combination of relativistic reflection and the effects of a warm corona at the surface of the accretion disc. Detailed examination of the soft excess can therefore constrain models
Externí odkaz:
http://arxiv.org/abs/2404.03040