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On the correlation between optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017. / Уголькова, Любовь; Шимановская, Е.; Ларионов, Валерий Михайлович; Савченко, Сергей Сергеевич; Гришина, Татьяна Сергеевна; Ежкова, О.; Копацкая, Евгения Николаевна; Ларионова, Елена Геннадиевна; Ларионова, Людмила Васильевна; Морозова, Дарья Адиковна; Никифорова, Анна Алексеевна; Троицкий, Иван Станиславович.

ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES: Proceedings of the VAK-2021 conference, Aug 23–28, 2021. 2022. стр. 404-406.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции › Рецензирование

Harvard

Уголькова, Л, Шимановская, Е, Ларионов, ВМ, Савченко, СС, Гришина, ТС, Ежкова, О, Копацкая, ЕН, Ларионова, ЕГ, Ларионова, ЛВ, Морозова, ДА, Никифорова, АА & Троицкий, ИС 2022, On the correlation between optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017. в ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES: Proceedings of the VAK-2021 conference, Aug 23–28, 2021. стр. 404-406, ВСЕРОССИЙСКАЯ АСТРОНОМИЧЕСКАЯ КОНФЕРЕНЦИЯ — 2021, Москва, Российская Федерация, 23/08/21. https://doi.org/10.51194/VAK2021.2022.1.1.166

APA

Уголькова, Л., Шимановская, Е., Ларионов, В. М., Савченко, С. С., Гришина, Т. С., Ежкова, О., Копацкая, Е. Н., Ларионова, Е. Г., Ларионова, Л. В., Морозова, Д. А., Никифорова, А. А., & Троицкий, И. С. (2022). On the correlation between optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017. в ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES: Proceedings of the VAK-2021 conference, Aug 23–28, 2021 (стр. 404-406) https://doi.org/10.51194/VAK2021.2022.1.1.166

Vancouver

Уголькова Л, Шимановская Е, Ларионов ВМ, Савченко СС, Гришина ТС, Ежкова О и пр. On the correlation between optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017. в ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES: Proceedings of the VAK-2021 conference, Aug 23–28, 2021. 2022. стр. 404-406 https://doi.org/10.51194/VAK2021.2022.1.1.166

Author

Уголькова, Любовь ; Шимановская, Е. ; Ларионов, Валерий Михайлович ; Савченко, Сергей Сергеевич ; Гришина, Татьяна Сергеевна ; Ежкова, О. ; Копацкая, Евгения Николаевна ; Ларионова, Елена Геннадиевна ; Ларионова, Людмила Васильевна ; Морозова, Дарья Адиковна ; Никифорова, Анна Алексеевна ; Троицкий, Иван Станиславович. / On the correlation between optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017. ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES: Proceedings of the VAK-2021 conference, Aug 23–28, 2021. 2022. стр. 404-406

BibTeX

@inproceedings{7cbca5d7a8e24f47a4fdaa09536e77ce,
title = "On the correlation between optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017",
abstract = "The correlation of optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017 isanalyzed. The light curves have a complex structure, especially during the period of maximum radiation in 2014, when theactivity in the form of a series of 4-5 small flares is observed. The cross-correlation functions exhibit almost zero lag betweenBVR and γ-ray emission at different periods of the long-term flares. This suggests that optical and γ-ray emission come fromapproximately the same location (probably the base of the jet) and are physically connected. In general, optical emission lagsbehind gamma radiation except a few cases. It is assumed that both synchrotron radiation and inverse Compton scatteringby relativistic electrons and protons, which is typical for strong flares, are present. The rotation of γ-ray radiation regionrelative to optical one is supposed.",
author = "Любовь Уголькова and Е. Шимановская and Ларионов, {Валерий Михайлович} and Савченко, {Сергей Сергеевич} and Гришина, {Татьяна Сергеевна} and О. Ежкова and Копацкая, {Евгения Николаевна} and Ларионова, {Елена Геннадиевна} and Ларионова, {Людмила Васильевна} and Морозова, {Дарья Адиковна} and Никифорова, {Анна Алексеевна} and Троицкий, {Иван Станиславович}",
year = "2022",
month = feb,
day = "22",
doi = "10.51194/VAK2021.2022.1.1.166",
language = "English",
pages = "404--406",
booktitle = "ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES",
note = "Всероссийская астрономическая конференция 2021 {"}Астрономия в эпоху многоканальных исследований{"}, ВАК-2021 ; Conference date: 23-08-2021 Through 28-08-2021",
url = "https://www.vak2021.ru/, https://www.vak2021.ru, https://www.vak2021.ru/timetable/",

}

RIS

TY - GEN

T1 - On the correlation between optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017

AU - Уголькова, Любовь

AU - Шимановская, Е.

AU - Ларионов, Валерий Михайлович

AU - Савченко, Сергей Сергеевич

AU - Гришина, Татьяна Сергеевна

AU - Ежкова, О.

AU - Копацкая, Евгения Николаевна

AU - Ларионова, Елена Геннадиевна

AU - Ларионова, Людмила Васильевна

AU - Морозова, Дарья Адиковна

AU - Никифорова, Анна Алексеевна

AU - Троицкий, Иван Станиславович

PY - 2022/2/22

Y1 - 2022/2/22

N2 - The correlation of optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017 isanalyzed. The light curves have a complex structure, especially during the period of maximum radiation in 2014, when theactivity in the form of a series of 4-5 small flares is observed. The cross-correlation functions exhibit almost zero lag betweenBVR and γ-ray emission at different periods of the long-term flares. This suggests that optical and γ-ray emission come fromapproximately the same location (probably the base of the jet) and are physically connected. In general, optical emission lagsbehind gamma radiation except a few cases. It is assumed that both synchrotron radiation and inverse Compton scatteringby relativistic electrons and protons, which is typical for strong flares, are present. The rotation of γ-ray radiation regionrelative to optical one is supposed.

AB - The correlation of optical and γ-ray emission of the blazar 3C 454.3 during the multi-wavelength flare from 2012 to 2017 isanalyzed. The light curves have a complex structure, especially during the period of maximum radiation in 2014, when theactivity in the form of a series of 4-5 small flares is observed. The cross-correlation functions exhibit almost zero lag betweenBVR and γ-ray emission at different periods of the long-term flares. This suggests that optical and γ-ray emission come fromapproximately the same location (probably the base of the jet) and are physically connected. In general, optical emission lagsbehind gamma radiation except a few cases. It is assumed that both synchrotron radiation and inverse Compton scatteringby relativistic electrons and protons, which is typical for strong flares, are present. The rotation of γ-ray radiation regionrelative to optical one is supposed.

UR - https://www.mendeley.com/catalogue/02c3eb8d-a0ee-327c-818b-dca073e2476a/

UR - https://www.mendeley.com/catalogue/02c3eb8d-a0ee-327c-818b-dca073e2476a/

U2 - 10.51194/VAK2021.2022.1.1.166

DO - 10.51194/VAK2021.2022.1.1.166

M3 - Conference contribution

SP - 404

EP - 406

BT - ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES

T2 - Всероссийская астрономическая конференция 2021 "Астрономия в эпоху многоканальных исследований"

Y2 - 23 August 2021 through 28 August 2021

ER -

ID: 93575687