On the TeV gamma-ray and X-ray correlations exhibited in high-energy peaked BL Lacs: Mrk 501 and 1ES 1959+650

被引：0
|
作者：
Osorio, Mabel [1 ,2 ]
Sacahui, Rodrigo [1 ]
Magdalena Gonzalez, M. [2 ]
Fraija, Nissim [2 ]
Garcia-Gonzalez, Jose Andres [3 ]
机构：
[1] USAC, Inst Invest Ciencias Fis & Matemat, ECFM, Guatemala City, Guatemala
[2] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City, Mexico
[3] Univ Nacl Autonoma Mexico, Inst Fis, Mexico City, Mexico
来源：
36TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2019 | 2021年
关键词：
MULTIWAVELENGTH OBSERVATIONS; FLARE;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The spectral energy distribution (SED) of blazars is generally understood through the standard one-zone synchrotron self-Compton (SSC) model, where a strong correlation between X-ray and TeV gamma-ray fluxes is expected. Recently, for Mrk 421 the correlation was confirmed and interpreted within the SSC model arguing that a description of the correlation up to large flux values considerably restricts the value of the magnetic field under the assumption of an electron spectral index independent of the flux state. In this work, we extend the analysis done on Mrk 421 for other two high-energy peaked BL Lacs: Mrk 501 and 1ES 1959+650.
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页数：8
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