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  • Determining the origin of the X-ray emission in blazars through multiwavelength polarization
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Determining the origin of the X-ray emission in blazars through multiwavelength polarization

Fuente: arXiv
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Bibliographic Details
Main Authors: Liodakis, Ioannis, Zhang, Haocheng, Boula, Stella, Middei, Riccardo, Otero-Santos, Jorge, Blinov, Dmitry, Agudo, Iván, Böttcher, Markus, Chen, Chien-Ting, Ehlert, Steven R., Jorstad, Svetlana G., Kaaret, Philip, Krawczynski, Henric, Peirson, Abel L., Romani, Roger W., Tavecchio, Fabrizio, Weisskopf, Martin C., Kouch, Pouya M., Lindfors, Elina, Nilsson, Kari, McCall, Callum, Jermak, Helen E., Steele, Iain A., Myserlis, Ioannis, Gurwell, Mark, Keating, Garrett K., Rao, Ramprasad, Kang, Sincheol, Lee, Sang-Sung, Kim, Sanghyun, Cheong, Whee Yeon, Jeong, Hyeon-Woo, Angelakis, Emmanouil, Kraus, Alexander, Aceituno, Francisco José, Bonnoli, Giacomo, Casanova, Víctor, Escudero, Juan, Agís-González, Beatriz, Morcuende, Daniel, Sota, Alfredo, Bachev, Rumen, Grishina, Tatiana S., Kopatskaya, Evgenia N., Larionova, Elena G., Morozova, Daria A., Savchenko, Sergey S., Shishkina, Ekaterina V., Troitskiy, Ivan S., Troitskaya, Yulia V., Vasilyev, Andrey A.
Format: Preprint
Published: 2025
Subjects:
High Energy Astrophysical Phenomena
Online Access:
Acceder al recurso
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