Broadband spectro-temporal study on blazar TXS 1700+685

نویسندگان

چکیده

We attempt to present a multiwavelength variability and correlation study as well detailed multi-waveband spectral characteristics of the May 2021 $\gamma$-ray flare blazar source TXS 1700+685. The multi-wavelength observation from \textit{Fermi}-LAT, \textit{Swift}-XRT/UVOT radio archival data are used for our spectro-temporal investigation. estimate time-scale flux doubling time in different flaring regions detected \textit{Fermi}-LAT shortest is put constraint on minimum Doppler factor size emission region. have statistically significant quasi-periodic oscillation feature (QPO) at $\sim$ 17 days. broad-band satisfactorily represented during its state with leptonic synchrotron inverse Compton component. From broadband modeling, we observe external Comptonization seed photons originating broad line region be dominant compared dusty torus. This further supported by fact that also found residing within BLR. equipartition value implies energy density magnetic field jet comoving frame weak, reflected low power corresponding component jet. In order produce high hump, need injection large population electrons and/or presence strong field; later sub-dominant case. flat rising steep falling profile SED break or curvature 1 GeV commensuration flat-spectrum quasar (FSRQ) nature source.

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2022

ISSN: ['0035-8711', '1365-8711', '1365-2966']

DOI: https://doi.org/10.1093/mnras/stac2068