X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304

We reviewed X-ray flux and spectral variability properties studied to date by various X-ray satellites for Mrk 421 and PKS 2155-304, which are TeV emitting blazars. Mrk 421 and PKS 2155-304 are the most X-ray luminous blazars in the northern and southern hemispheres, respectively. Blazars show flux...

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Main Author: Alok C. Gupta
Format: Article
Language:English
Published: MDPI AG 2020-09-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/8/3/64
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author Alok C. Gupta
author_facet Alok C. Gupta
author_sort Alok C. Gupta
collection DOAJ
description We reviewed X-ray flux and spectral variability properties studied to date by various X-ray satellites for Mrk 421 and PKS 2155-304, which are TeV emitting blazars. Mrk 421 and PKS 2155-304 are the most X-ray luminous blazars in the northern and southern hemispheres, respectively. Blazars show flux and spectral variabilities in the complete electromagnetic spectrum on diverse timescales ranging from a few minutes to hours, days, weeks, months and even several years. The flux and spectral variability on different timescales can be used to constrain the size of the emitting region, estimate the super massive black hole mass, find the dominant emission mechanism in the close vicinity of the super massive black hole, search for quasi-periodic oscillations in time series data and several other physical parameters of blazars. Flux and spectral variability is also a dominant tool to explain jet as well as disk emission from blazars at different epochs of observations.
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spelling doaj.art-221e0735c43b47ff9b5d94ae53d1273b2023-11-20T12:36:06ZengMDPI AGGalaxies2075-44342020-09-01836410.3390/galaxies8030064X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304Alok C. Gupta0Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263001, IndiaWe reviewed X-ray flux and spectral variability properties studied to date by various X-ray satellites for Mrk 421 and PKS 2155-304, which are TeV emitting blazars. Mrk 421 and PKS 2155-304 are the most X-ray luminous blazars in the northern and southern hemispheres, respectively. Blazars show flux and spectral variabilities in the complete electromagnetic spectrum on diverse timescales ranging from a few minutes to hours, days, weeks, months and even several years. The flux and spectral variability on different timescales can be used to constrain the size of the emitting region, estimate the super massive black hole mass, find the dominant emission mechanism in the close vicinity of the super massive black hole, search for quasi-periodic oscillations in time series data and several other physical parameters of blazars. Flux and spectral variability is also a dominant tool to explain jet as well as disk emission from blazars at different epochs of observations.https://www.mdpi.com/2075-4434/8/3/64BL Lac objectsindividualMrk 421PKS 2155-304 galaxiesactive galaxiesjets radiation mechanisms
spellingShingle Alok C. Gupta
X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304
Galaxies
BL Lac objects
individual
Mrk 421
PKS 2155-304 galaxies
active galaxies
jets radiation mechanisms
title X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304
title_full X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304
title_fullStr X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304
title_full_unstemmed X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304
title_short X-ray Flux and Spectral Variability of the TeV Blazars Mrk 421 and PKS 2155-304
title_sort x ray flux and spectral variability of the tev blazars mrk 421 and pks 2155 304
topic BL Lac objects
individual
Mrk 421
PKS 2155-304 galaxies
active galaxies
jets radiation mechanisms
url https://www.mdpi.com/2075-4434/8/3/64
work_keys_str_mv AT alokcgupta xrayfluxandspectralvariabilityofthetevblazarsmrk421andpks2155304