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Variability of the Blazar B1308+326 in 2011-2018. / Hagen-Thorn, V. A.; Morozova, D. A.; Hagen-Thorn, E. I.; Savchenko, S. S.; Troitsky, I.S.; Shaliapina, L. V.; Volkov, E. V.

в: Astronomy Reports, Том 64, № 8, 01.08.2020, стр. 663-671.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Hagen-Thorn, VA, Morozova, DA, Hagen-Thorn, EI, Savchenko, SS, Troitsky, IS, Shaliapina, LV & Volkov, EV 2020, 'Variability of the Blazar B1308+326 in 2011-2018', Astronomy Reports, Том. 64, № 8, стр. 663-671. https://doi.org/10.1134/S1063772920080041

APA

Hagen-Thorn, V. A., Morozova, D. A., Hagen-Thorn, E. I., Savchenko, S. S., Troitsky, I. S., Shaliapina, L. V., & Volkov, E. V. (2020). Variability of the Blazar B1308+326 in 2011-2018. Astronomy Reports, 64(8), 663-671. https://doi.org/10.1134/S1063772920080041

Vancouver

Hagen-Thorn VA, Morozova DA, Hagen-Thorn EI, Savchenko SS, Troitsky IS, Shaliapina LV и пр. Variability of the Blazar B1308+326 in 2011-2018. Astronomy Reports. 2020 Авг. 1;64(8):663-671. https://doi.org/10.1134/S1063772920080041

Author

Hagen-Thorn, V. A. ; Morozova, D. A. ; Hagen-Thorn, E. I. ; Savchenko, S. S. ; Troitsky, I.S. ; Shaliapina, L. V. ; Volkov, E. V. / Variability of the Blazar B1308+326 in 2011-2018. в: Astronomy Reports. 2020 ; Том 64, № 8. стр. 663-671.

BibTeX

@article{ced9b9d1744f4fa28a24a625d16823ff,
title = "Variability of the Blazar B1308+326 in 2011-2018",
abstract = "The monitoring results of the blazar B1308+326 in the optical and radio bands in 2011-2018 are presented and analyzed. An optical flare of the object associated with the passage of revealed superluminal components through the radio core, coinciding in time with a γ-ray outburst, as well as outbursts at 43 GHz, were detected. The photometric variability is explained by a variable component with a constant at average power-law relative energy distribution in the spectrum (Fν ~ ν-1.6). This fact, as well as the high observed degree of polarization (up to 40%), indicates its synchrotron nature. Separate sources of polarized radiation with a high degree of polarization and a direction either parallel or perpendicular to the direction of the jet are distinguished, which gives information about the magnetic field's direction in the jet during outbursts and allows us to make a conclusion for their appearance: the passage of a shock wave over the jet or the appearance of radiating electronic ensembles.",
keywords = "OBJECT, OUTBURST, PHOTOMETRY, POLARIZATION",
author = "Hagen-Thorn, {V. A.} and Morozova, {D. A.} and Hagen-Thorn, {E. I.} and Savchenko, {S. S.} and I.S. Troitsky and Shaliapina, {L. V.} and Volkov, {E. V.}",
note = "Publisher Copyright: {\textcopyright} 2020, Pleiades Publishing, Ltd.",
year = "2020",
month = aug,
day = "1",
doi = "10.1134/S1063772920080041",
language = "English",
volume = "64",
pages = "663--671",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "8",

}

RIS

TY - JOUR

T1 - Variability of the Blazar B1308+326 in 2011-2018

AU - Hagen-Thorn, V. A.

AU - Morozova, D. A.

AU - Hagen-Thorn, E. I.

AU - Savchenko, S. S.

AU - Troitsky, I.S.

AU - Shaliapina, L. V.

AU - Volkov, E. V.

N1 - Publisher Copyright: © 2020, Pleiades Publishing, Ltd.

PY - 2020/8/1

Y1 - 2020/8/1

N2 - The monitoring results of the blazar B1308+326 in the optical and radio bands in 2011-2018 are presented and analyzed. An optical flare of the object associated with the passage of revealed superluminal components through the radio core, coinciding in time with a γ-ray outburst, as well as outbursts at 43 GHz, were detected. The photometric variability is explained by a variable component with a constant at average power-law relative energy distribution in the spectrum (Fν ~ ν-1.6). This fact, as well as the high observed degree of polarization (up to 40%), indicates its synchrotron nature. Separate sources of polarized radiation with a high degree of polarization and a direction either parallel or perpendicular to the direction of the jet are distinguished, which gives information about the magnetic field's direction in the jet during outbursts and allows us to make a conclusion for their appearance: the passage of a shock wave over the jet or the appearance of radiating electronic ensembles.

AB - The monitoring results of the blazar B1308+326 in the optical and radio bands in 2011-2018 are presented and analyzed. An optical flare of the object associated with the passage of revealed superluminal components through the radio core, coinciding in time with a γ-ray outburst, as well as outbursts at 43 GHz, were detected. The photometric variability is explained by a variable component with a constant at average power-law relative energy distribution in the spectrum (Fν ~ ν-1.6). This fact, as well as the high observed degree of polarization (up to 40%), indicates its synchrotron nature. Separate sources of polarized radiation with a high degree of polarization and a direction either parallel or perpendicular to the direction of the jet are distinguished, which gives information about the magnetic field's direction in the jet during outbursts and allows us to make a conclusion for their appearance: the passage of a shock wave over the jet or the appearance of radiating electronic ensembles.

KW - OBJECT

KW - OUTBURST

KW - PHOTOMETRY

KW - POLARIZATION

UR - http://www.scopus.com/inward/record.url?scp=85089997064&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/7d3d2089-6bf7-3af5-8e77-d9f7ba43a500/

U2 - 10.1134/S1063772920080041

DO - 10.1134/S1063772920080041

M3 - Article

VL - 64

SP - 663

EP - 671

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 8

ER -

ID: 64693711