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Variations of the Blazar AO 0235+164 in 2006–2015. / Hagen-Thorn, V. A.; Larionov, V. M.; Morozova, D. A.; Arkharov, A. A.; Hagen-Thorn, E. I.; Shablovinskaya, E. S.; Prokop’eva, M. S.; Yakovleva, V. A.

In: Astronomy Reports, Vol. 62, No. 2, 01.02.2018, p. 103-115.

Research output: Contribution to journal › Article › peer-review

Harvard

Hagen-Thorn, VA, Larionov, VM, Morozova, DA, Arkharov, AA, Hagen-Thorn, EI, Shablovinskaya, ES, Prokop’eva, MS & Yakovleva, VA 2018, 'Variations of the Blazar AO 0235+164 in 2006–2015', Astronomy Reports, vol. 62, no. 2, pp. 103-115. https://doi.org/10.1134/S106377291802004X

APA

Hagen-Thorn, V. A., Larionov, V. M., Morozova, D. A., Arkharov, A. A., Hagen-Thorn, E. I., Shablovinskaya, E. S., Prokop’eva, M. S., & Yakovleva, V. A. (2018). Variations of the Blazar AO 0235+164 in 2006–2015. Astronomy Reports, 62(2), 103-115. https://doi.org/10.1134/S106377291802004X

Vancouver

Hagen-Thorn VA, Larionov VM, Morozova DA, Arkharov AA, Hagen-Thorn EI, Shablovinskaya ES et al. Variations of the Blazar AO 0235+164 in 2006–2015. Astronomy Reports. 2018 Feb 1;62(2):103-115. https://doi.org/10.1134/S106377291802004X

Author

Hagen-Thorn, V. A. ; Larionov, V. M. ; Morozova, D. A. ; Arkharov, A. A. ; Hagen-Thorn, E. I. ; Shablovinskaya, E. S. ; Prokop’eva, M. S. ; Yakovleva, V. A. / Variations of the Blazar AO 0235+164 in 2006–2015. In: Astronomy Reports. 2018 ; Vol. 62, No. 2. pp. 103-115.

BibTeX

@article{9f317773df4448498f15d7ef8bdb7db4,
title = "Variations of the Blazar AO 0235+164 in 2006–2015",
abstract = "The results of optical, radio, and gamma-ray observations of the blazar AO 0235+16 are presented, including photometric (BV RIJHK) and polarimetric (R)monitoring carried out at St. Petersburg State University and the Central (Pulkovo) Astronomical Observatory in 2007–2015, 43 GHz Very Long Baseline Interferometry radio observations processed at Boston University, and a gamma-ray light curve based on observationswith the Fermi space observatory are presented. Two strong outbursts were detected. The relative spectral energy distributions of the variable components responsible for the outbursts are determined; these follow power laws, but with different spectral indices. The degree of polarization was high in both outbursts; only an average relationship between the brightness and polarization can be found. There was no time lag between the variations in the optical and gamma-ray, suggesting that the sources of the radiation in the optical and gamma-ray are located in the same region of the jet.",
author = "Hagen-Thorn, {V. A.} and Larionov, {V. M.} and Morozova, {D. A.} and Arkharov, {A. A.} and Hagen-Thorn, {E. I.} and Shablovinskaya, {E. S.} and Prokop{\textquoteright}eva, {M. S.} and Yakovleva, {V. A.}",
note = "Publisher Copyright: {\textcopyright} 2018, Pleiades Publishing, Ltd.",
year = "2018",
month = feb,
day = "1",
doi = "10.1134/S106377291802004X",
language = "English",
volume = "62",
pages = "103--115",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "2",

}

RIS

TY - JOUR

T1 - Variations of the Blazar AO 0235+164 in 2006–2015

AU - Hagen-Thorn, V. A.

AU - Larionov, V. M.

AU - Morozova, D. A.

AU - Arkharov, A. A.

AU - Hagen-Thorn, E. I.

AU - Shablovinskaya, E. S.

AU - Prokop’eva, M. S.

AU - Yakovleva, V. A.

N1 - Publisher Copyright: © 2018, Pleiades Publishing, Ltd.

PY - 2018/2/1

Y1 - 2018/2/1

N2 - The results of optical, radio, and gamma-ray observations of the blazar AO 0235+16 are presented, including photometric (BV RIJHK) and polarimetric (R)monitoring carried out at St. Petersburg State University and the Central (Pulkovo) Astronomical Observatory in 2007–2015, 43 GHz Very Long Baseline Interferometry radio observations processed at Boston University, and a gamma-ray light curve based on observationswith the Fermi space observatory are presented. Two strong outbursts were detected. The relative spectral energy distributions of the variable components responsible for the outbursts are determined; these follow power laws, but with different spectral indices. The degree of polarization was high in both outbursts; only an average relationship between the brightness and polarization can be found. There was no time lag between the variations in the optical and gamma-ray, suggesting that the sources of the radiation in the optical and gamma-ray are located in the same region of the jet.

AB - The results of optical, radio, and gamma-ray observations of the blazar AO 0235+16 are presented, including photometric (BV RIJHK) and polarimetric (R)monitoring carried out at St. Petersburg State University and the Central (Pulkovo) Astronomical Observatory in 2007–2015, 43 GHz Very Long Baseline Interferometry radio observations processed at Boston University, and a gamma-ray light curve based on observationswith the Fermi space observatory are presented. Two strong outbursts were detected. The relative spectral energy distributions of the variable components responsible for the outbursts are determined; these follow power laws, but with different spectral indices. The degree of polarization was high in both outbursts; only an average relationship between the brightness and polarization can be found. There was no time lag between the variations in the optical and gamma-ray, suggesting that the sources of the radiation in the optical and gamma-ray are located in the same region of the jet.

UR - http://www.scopus.com/inward/record.url?scp=85043462149&partnerID=8YFLogxK

U2 - 10.1134/S106377291802004X

DO - 10.1134/S106377291802004X

M3 - Article

AN - SCOPUS:85043462149

VL - 62

SP - 103

EP - 115

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 2

ER -

ID: 86248546