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Variability of the Blazar 4C 38.41 in 2006–2017. / Hagen-Thorn, V. A.; Troitskaya, Yu V.; Hagen-Thorn, E.I.; Troitsky, I. S.; Savchenko, S. S.; Arharov, A. A.; Efimova, N. V.; Klimanov, S. K.; Volkov, E. V.

в: Astronomy Reports, Том 63, № 5, 01.05.2019, стр. 378-390.

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

Harvard

Hagen-Thorn, VA, Troitskaya, YV, Hagen-Thorn, EI, Troitsky, IS, Savchenko, SS, Arharov, AA, Efimova, NV, Klimanov, SK & Volkov, EV 2019, 'Variability of the Blazar 4C 38.41 in 2006–2017', Astronomy Reports, Том. 63, № 5, стр. 378-390. https://doi.org/10.1134/S1063772919040036

APA

Hagen-Thorn, V. A., Troitskaya, Y. V., Hagen-Thorn, E. I., Troitsky, I. S., Savchenko, S. S., Arharov, A. A., Efimova, N. V., Klimanov, S. K., & Volkov, E. V. (2019). Variability of the Blazar 4C 38.41 in 2006–2017. Astronomy Reports, 63(5), 378-390. https://doi.org/10.1134/S1063772919040036

Vancouver

Hagen-Thorn VA, Troitskaya YV, Hagen-Thorn EI, Troitsky IS, Savchenko SS, Arharov AA и пр. Variability of the Blazar 4C 38.41 in 2006–2017. Astronomy Reports. 2019 Май 1;63(5):378-390. https://doi.org/10.1134/S1063772919040036

Author

Hagen-Thorn, V. A. ; Troitskaya, Yu V. ; Hagen-Thorn, E.I. ; Troitsky, I. S. ; Savchenko, S. S. ; Arharov, A. A. ; Efimova, N. V. ; Klimanov, S. K. ; Volkov, E. V. / Variability of the Blazar 4C 38.41 in 2006–2017. в: Astronomy Reports. 2019 ; Том 63, № 5. стр. 378-390.

BibTeX

@article{0d7e0f04f8494fab89767e64c215b268,
title = "Variability of the Blazar 4C 38.41 in 2006–2017",
abstract = "The results of multicolor photometric and polarization observations of the blazar 4C 38.41 (Q 1633+382) performed at St. Petersburg State University, the Pulkovo Astronomical Observatory of the Russian Academy of Sciences, Boston University, and Steward Observatory in 2006–2017 are analyzed. Separate variable sources responsible for the observed activity are distinguished, whose power-lawspectra and high degree of polarization confirm their synchrotron nature. The observed color variability of the object (redder when brighter) can be explained by an increase in the contribution to the total emission of a red component with variable flux and a constant relative spectral energy distribution. A close correlation between the optical and gamma-ray light curves is identified, suggesting the same location of the variable sources responsible for the radiation in these bands.",
author = "Hagen-Thorn, {V. A.} and Troitskaya, {Yu V.} and E.I. Hagen-Thorn and Troitsky, {I. S.} and Savchenko, {S. S.} and Arharov, {A. A.} and Efimova, {N. V.} and Klimanov, {S. K.} and Volkov, {E. V.}",
year = "2019",
month = may,
day = "1",
doi = "10.1134/S1063772919040036",
language = "English",
volume = "63",
pages = "378--390",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "5",

}

RIS

TY - JOUR

T1 - Variability of the Blazar 4C 38.41 in 2006–2017

AU - Hagen-Thorn, V. A.

AU - Troitskaya, Yu V.

AU - Hagen-Thorn, E.I.

AU - Troitsky, I. S.

AU - Savchenko, S. S.

AU - Arharov, A. A.

AU - Efimova, N. V.

AU - Klimanov, S. K.

AU - Volkov, E. V.

PY - 2019/5/1

Y1 - 2019/5/1

N2 - The results of multicolor photometric and polarization observations of the blazar 4C 38.41 (Q 1633+382) performed at St. Petersburg State University, the Pulkovo Astronomical Observatory of the Russian Academy of Sciences, Boston University, and Steward Observatory in 2006–2017 are analyzed. Separate variable sources responsible for the observed activity are distinguished, whose power-lawspectra and high degree of polarization confirm their synchrotron nature. The observed color variability of the object (redder when brighter) can be explained by an increase in the contribution to the total emission of a red component with variable flux and a constant relative spectral energy distribution. A close correlation between the optical and gamma-ray light curves is identified, suggesting the same location of the variable sources responsible for the radiation in these bands.

AB - The results of multicolor photometric and polarization observations of the blazar 4C 38.41 (Q 1633+382) performed at St. Petersburg State University, the Pulkovo Astronomical Observatory of the Russian Academy of Sciences, Boston University, and Steward Observatory in 2006–2017 are analyzed. Separate variable sources responsible for the observed activity are distinguished, whose power-lawspectra and high degree of polarization confirm their synchrotron nature. The observed color variability of the object (redder when brighter) can be explained by an increase in the contribution to the total emission of a red component with variable flux and a constant relative spectral energy distribution. A close correlation between the optical and gamma-ray light curves is identified, suggesting the same location of the variable sources responsible for the radiation in these bands.

UR - http://www.scopus.com/inward/record.url?scp=85065205723&partnerID=8YFLogxK

U2 - 10.1134/S1063772919040036

DO - 10.1134/S1063772919040036

M3 - Article

AN - SCOPUS:85065205723

VL - 63

SP - 378

EP - 390

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 5

ER -

ID: 42191852