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Behaviour of the blazar CTA 102 during two giant outbursts. / Larionov, Valeri M.; Jorstad, Svetlana G.; Marscher, Alan P.; Smith, Paul S.; Savchenko, Sergey; Morozova, Daria; Grishina, Tatiana; Kopatskaya, Evgenia; Larionova, Liudmila; Larionova, Elena; Mokrushina, Anna; Troitsky, Ivan; Troitskaya, Yulia; Borman, George.

в: Galaxies, Том 5, № 4, 91, 30.11.2017.

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

Harvard

Larionov, VM, Jorstad, SG, Marscher, AP, Smith, PS, Savchenko, S, Morozova, D, Grishina, T, Kopatskaya, E, Larionova, L, Larionova, E, Mokrushina, A, Troitsky, I, Troitskaya, Y & Borman, G 2017, 'Behaviour of the blazar CTA 102 during two giant outbursts', Galaxies, Том. 5, № 4, 91. https://doi.org/10.3390/galaxies5040091

APA

Larionov, V. M., Jorstad, S. G., Marscher, A. P., Smith, P. S., Savchenko, S., Morozova, D., Grishina, T., Kopatskaya, E., Larionova, L., Larionova, E., Mokrushina, A., Troitsky, I., Troitskaya, Y., & Borman, G. (2017). Behaviour of the blazar CTA 102 during two giant outbursts. Galaxies, 5(4), [91]. https://doi.org/10.3390/galaxies5040091

Vancouver

Larionov VM, Jorstad SG, Marscher AP, Smith PS, Savchenko S, Morozova D и пр. Behaviour of the blazar CTA 102 during two giant outbursts. Galaxies. 2017 Нояб. 30;5(4). 91. https://doi.org/10.3390/galaxies5040091

Author

Larionov, Valeri M. ; Jorstad, Svetlana G. ; Marscher, Alan P. ; Smith, Paul S. ; Savchenko, Sergey ; Morozova, Daria ; Grishina, Tatiana ; Kopatskaya, Evgenia ; Larionova, Liudmila ; Larionova, Elena ; Mokrushina, Anna ; Troitsky, Ivan ; Troitskaya, Yulia ; Borman, George. / Behaviour of the blazar CTA 102 during two giant outbursts. в: Galaxies. 2017 ; Том 5, № 4.

BibTeX

@article{f758c63767204a1d89bd9131efcca9ec,
title = "Behaviour of the blazar CTA 102 during two giant outbursts",
abstract = "Blazar CTA 102 underwent exceptional optical and high-energy outbursts in 2012 and 2016-2017. We analyze its behaviour during these events, focusing on polarimetry as a tool that allows us to trace changes in the physical conditions and geometric configuration of the emission source close to the central black hole. We also use Fermi γ-ray data in conjunction with optical photometry in an effort to localize the origin of the outbursts.",
keywords = "Blazars, Methods of analysis, Photometry, Polarimetry",
author = "Larionov, {Valeri M.} and Jorstad, {Svetlana G.} and Marscher, {Alan P.} and Smith, {Paul S.} and Sergey Savchenko and Daria Morozova and Tatiana Grishina and Evgenia Kopatskaya and Liudmila Larionova and Elena Larionova and Anna Mokrushina and Ivan Troitsky and Yulia Troitskaya and George Borman",
year = "2017",
month = nov,
day = "30",
doi = "10.3390/galaxies5040091",
language = "English",
volume = "5",
journal = "Galaxies",
issn = "2075-4434",
publisher = "MDPI AG",
number = "4",

}

RIS

TY - JOUR

T1 - Behaviour of the blazar CTA 102 during two giant outbursts

AU - Larionov, Valeri M.

AU - Jorstad, Svetlana G.

AU - Marscher, Alan P.

AU - Smith, Paul S.

AU - Savchenko, Sergey

AU - Morozova, Daria

AU - Grishina, Tatiana

AU - Kopatskaya, Evgenia

AU - Larionova, Liudmila

AU - Larionova, Elena

AU - Mokrushina, Anna

AU - Troitsky, Ivan

AU - Troitskaya, Yulia

AU - Borman, George

PY - 2017/11/30

Y1 - 2017/11/30

N2 - Blazar CTA 102 underwent exceptional optical and high-energy outbursts in 2012 and 2016-2017. We analyze its behaviour during these events, focusing on polarimetry as a tool that allows us to trace changes in the physical conditions and geometric configuration of the emission source close to the central black hole. We also use Fermi γ-ray data in conjunction with optical photometry in an effort to localize the origin of the outbursts.

AB - Blazar CTA 102 underwent exceptional optical and high-energy outbursts in 2012 and 2016-2017. We analyze its behaviour during these events, focusing on polarimetry as a tool that allows us to trace changes in the physical conditions and geometric configuration of the emission source close to the central black hole. We also use Fermi γ-ray data in conjunction with optical photometry in an effort to localize the origin of the outbursts.

KW - Blazars

KW - Methods of analysis

KW - Photometry

KW - Polarimetry

UR - http://www.scopus.com/inward/record.url?scp=85036649398&partnerID=8YFLogxK

U2 - 10.3390/galaxies5040091

DO - 10.3390/galaxies5040091

M3 - Article

AN - SCOPUS:85036649398

VL - 5

JO - Galaxies

JF - Galaxies

SN - 2075-4434

IS - 4

M1 - 91

ER -

ID: 16273256