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Analysis of multicolor observations of 3C 66A in 1993-1998. / Hagen-Thorn, V. A.; Hagen-Thorn, A. V.; Jorstad, S. G.; Takalo, L. O.; Sillanpää, A.; Pursimo, T.; Boltwood, P.

в: Astrophysics, Том 44, № 3, 2001, стр. 283-291.

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

Harvard

Hagen-Thorn, VA, Hagen-Thorn, AV, Jorstad, SG, Takalo, LO, Sillanpää, A, Pursimo, T & Boltwood, P 2001, 'Analysis of multicolor observations of 3C 66A in 1993-1998', Astrophysics, Том. 44, № 3, стр. 283-291. https://doi.org/10.1023/A:1012809409416

APA

Hagen-Thorn, V. A., Hagen-Thorn, A. V., Jorstad, S. G., Takalo, L. O., Sillanpää, A., Pursimo, T., & Boltwood, P. (2001). Analysis of multicolor observations of 3C 66A in 1993-1998. Astrophysics, 44(3), 283-291. https://doi.org/10.1023/A:1012809409416

Vancouver

Hagen-Thorn VA, Hagen-Thorn AV, Jorstad SG, Takalo LO, Sillanpää A, Pursimo T и пр. Analysis of multicolor observations of 3C 66A in 1993-1998. Astrophysics. 2001;44(3):283-291. https://doi.org/10.1023/A:1012809409416

Author

Hagen-Thorn, V. A. ; Hagen-Thorn, A. V. ; Jorstad, S. G. ; Takalo, L. O. ; Sillanpää, A. ; Pursimo, T. ; Boltwood, P. / Analysis of multicolor observations of 3C 66A in 1993-1998. в: Astrophysics. 2001 ; Том 44, № 3. стр. 283-291.

BibTeX

@article{17055fd5558c4e5c88b4f2a7a5dbc26d,
title = "Analysis of multicolor observations of 3C 66A in 1993-1998",
abstract = "The results of multicolor observations of the blazar 3C 66A, obtained in the course of the project OJ-94, are analyzed. It is established that the energy distribution of the variable source in the optical and IR ranges can be represented, on the average, by a power law: Fv ∝ v-0.92. Since the blazar's emission is strongly polarized, there is no doubt of the synchrotron nature of the variable source responsible for the blazar's activity.",
author = "Hagen-Thorn, {V. A.} and Hagen-Thorn, {A. V.} and Jorstad, {S. G.} and Takalo, {L. O.} and A. Sillanp{\"a}{\"a} and T. Pursimo and P. Boltwood",
year = "2001",
doi = "10.1023/A:1012809409416",
language = "English",
volume = "44",
pages = "283--291",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "3",

}

RIS

TY - JOUR

T1 - Analysis of multicolor observations of 3C 66A in 1993-1998

AU - Hagen-Thorn, V. A.

AU - Hagen-Thorn, A. V.

AU - Jorstad, S. G.

AU - Takalo, L. O.

AU - Sillanpää, A.

AU - Pursimo, T.

AU - Boltwood, P.

PY - 2001

Y1 - 2001

N2 - The results of multicolor observations of the blazar 3C 66A, obtained in the course of the project OJ-94, are analyzed. It is established that the energy distribution of the variable source in the optical and IR ranges can be represented, on the average, by a power law: Fv ∝ v-0.92. Since the blazar's emission is strongly polarized, there is no doubt of the synchrotron nature of the variable source responsible for the blazar's activity.

AB - The results of multicolor observations of the blazar 3C 66A, obtained in the course of the project OJ-94, are analyzed. It is established that the energy distribution of the variable source in the optical and IR ranges can be represented, on the average, by a power law: Fv ∝ v-0.92. Since the blazar's emission is strongly polarized, there is no doubt of the synchrotron nature of the variable source responsible for the blazar's activity.

UR - http://www.scopus.com/inward/record.url?scp=0041794176&partnerID=8YFLogxK

U2 - 10.1023/A:1012809409416

DO - 10.1023/A:1012809409416

M3 - Review article

AN - SCOPUS:0041794176

VL - 44

SP - 283

EP - 291

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 3

ER -

ID: 88371298