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Multifrequency polarization properties of blazars. / Jorstad, S.; Marscher, A.; Stevens, J.; Smith, P.; Forster, J.; Lister, M.; Stirling, A.; Gómez, J.; Cawthorne, T.; Gear, W.; Robson, I.

в: Chinese Journal of Astronomy and Astrophysics, Том 6, № SUPPL. 1, 2006, стр. 247-252.

Результаты исследований: Научные публикации в периодических изданиях › статья в журнале по материалам конференции › Рецензирование

Harvard

Jorstad, S, Marscher, A, Stevens, J, Smith, P, Forster, J, Lister, M, Stirling, A, Gómez, J, Cawthorne, T, Gear, W & Robson, I 2006, 'Multifrequency polarization properties of blazars', Chinese Journal of Astronomy and Astrophysics, Том. 6, № SUPPL. 1, стр. 247-252. https://doi.org/10.1088/1009-9271/6/s1/31

APA

Jorstad, S., Marscher, A., Stevens, J., Smith, P., Forster, J., Lister, M., Stirling, A., Gómez, J., Cawthorne, T., Gear, W., & Robson, I. (2006). Multifrequency polarization properties of blazars. Chinese Journal of Astronomy and Astrophysics, 6(SUPPL. 1), 247-252. https://doi.org/10.1088/1009-9271/6/s1/31

Vancouver

Jorstad S, Marscher A, Stevens J, Smith P, Forster J, Lister M и пр. Multifrequency polarization properties of blazars. Chinese Journal of Astronomy and Astrophysics. 2006;6(SUPPL. 1):247-252. https://doi.org/10.1088/1009-9271/6/s1/31

Author

Jorstad, S. ; Marscher, A. ; Stevens, J. ; Smith, P. ; Forster, J. ; Lister, M. ; Stirling, A. ; Gómez, J. ; Cawthorne, T. ; Gear, W. ; Robson, I. / Multifrequency polarization properties of blazars. в: Chinese Journal of Astronomy and Astrophysics. 2006 ; Том 6, № SUPPL. 1. стр. 247-252.

BibTeX

@article{060b8f13f8a2482283387ee07d908891,
title = "Multifrequency polarization properties of blazars",
abstract = "We report preliminary results of a 3-year multifrequency polarization campaign of 15 AGNs of blazar type, including bimonthly total and polarized intensity imaging at 7 mm with the VLBA. We find that the sources have two different dependences of degree of polarization on wavelength: sub-mm peaked or straight {"}polarization spectra{"}. The fractional polarization of the latter group increases with frequency. All sources with sub-mm peak polarization (6 objects) have similar degree of polarization in the optical region and in the VLBA core. In high-optically polarized sources (5 objects) the EVPAs at all frequencies align with the pc-scale jet direction within the 1σ uncertainties. This implies that the high frequency emission is co-spatial with the VLBI core and/or transverse shocks in the jet.",
keywords = "3C 120), 3C 273, 3C 279, 3C 345, 3C 454.3), Active, BL Lac), CTA 102, Galaxies: BL Lacertae objects: individual (3C 66A, Galaxies: individual (3C 111, Galaxies: jet, Galaxies: quasars: individual (0420-014, OJ 287, PKS 1510-089",
author = "S. Jorstad and A. Marscher and J. Stevens and P. Smith and J. Forster and M. Lister and A. Stirling and J. G{\'o}mez and T. Cawthorne and W. Gear and I. Robson",
year = "2006",
doi = "10.1088/1009-9271/6/s1/31",
language = "English",
volume = "6",
pages = "247--252",
journal = "Chinese Journal of Astronomy and Astrophysics",
issn = "1009-9271",
publisher = "Kexue Chubaneshe/Science Press",
number = "SUPPL. 1",
note = "6th International Workshop on Multifrequency Behaviour of High Energy Cosmic Sources: Frascati Workshop 2005 ; Conference date: 23-05-2005 Through 28-05-2005",

}

RIS

TY - JOUR

T1 - Multifrequency polarization properties of blazars

AU - Jorstad, S.

AU - Marscher, A.

AU - Stevens, J.

AU - Smith, P.

AU - Forster, J.

AU - Lister, M.

AU - Stirling, A.

AU - Gómez, J.

AU - Cawthorne, T.

AU - Gear, W.

AU - Robson, I.

PY - 2006

Y1 - 2006

N2 - We report preliminary results of a 3-year multifrequency polarization campaign of 15 AGNs of blazar type, including bimonthly total and polarized intensity imaging at 7 mm with the VLBA. We find that the sources have two different dependences of degree of polarization on wavelength: sub-mm peaked or straight "polarization spectra". The fractional polarization of the latter group increases with frequency. All sources with sub-mm peak polarization (6 objects) have similar degree of polarization in the optical region and in the VLBA core. In high-optically polarized sources (5 objects) the EVPAs at all frequencies align with the pc-scale jet direction within the 1σ uncertainties. This implies that the high frequency emission is co-spatial with the VLBI core and/or transverse shocks in the jet.

AB - We report preliminary results of a 3-year multifrequency polarization campaign of 15 AGNs of blazar type, including bimonthly total and polarized intensity imaging at 7 mm with the VLBA. We find that the sources have two different dependences of degree of polarization on wavelength: sub-mm peaked or straight "polarization spectra". The fractional polarization of the latter group increases with frequency. All sources with sub-mm peak polarization (6 objects) have similar degree of polarization in the optical region and in the VLBA core. In high-optically polarized sources (5 objects) the EVPAs at all frequencies align with the pc-scale jet direction within the 1σ uncertainties. This implies that the high frequency emission is co-spatial with the VLBI core and/or transverse shocks in the jet.

KW - 3C 120)

KW - 3C 273

KW - 3C 279

KW - 3C 345

KW - 3C 454.3)

KW - Active

KW - BL Lac)

KW - CTA 102

KW - Galaxies: BL Lacertae objects: individual (3C 66A

KW - Galaxies: individual (3C 111

KW - Galaxies: jet

KW - Galaxies: quasars: individual (0420-014

KW - OJ 287

KW - PKS 1510-089

UR - http://www.scopus.com/inward/record.url?scp=84891838155&partnerID=8YFLogxK

U2 - 10.1088/1009-9271/6/s1/31

DO - 10.1088/1009-9271/6/s1/31

M3 - Conference article

AN - SCOPUS:84891838155

VL - 6

SP - 247

EP - 252

JO - Chinese Journal of Astronomy and Astrophysics

JF - Chinese Journal of Astronomy and Astrophysics

SN - 1009-9271

IS - SUPPL. 1

T2 - 6th International Workshop on Multifrequency Behaviour of High Energy Cosmic Sources: Frascati Workshop 2005

Y2 - 23 May 2005 through 28 May 2005

ER -

ID: 88374614