Constraining the magnetic field in the parsec-scale jets of the brightest Fermi blazars with multifrequency VLBI observations

K. V. Sokolovsky; Y. Y. Kovalev; A. P. Lobanov; T. Savolainen; A. B. Pushkarev; M. Kadler

Constraining the magnetic field in the parsec-scale jets of the brightest Fermi blazars with multifrequency VLBI observations

K. V. Sokolovsky, Y. Y. Kovalev, A. P. Lobanov, T. Savolainen, A. B. Pushkarev, M. Kadler

Max Planck Inst Radioastron, Max Planck Society

Tutkimustuotos: Artikkeli kirjassa/konferenssijulkaisussa › Conference article in proceedings › Scientific › vertaisarvioitu

Abstrakti

The spatially resolved broad-band spectroscopy with Very Long Baseline Interferometry (VLBI) is one of the few methods that can probe the physical conditions inside blazar jets. We report on measurements of the magnetic field strength in parsec-scale radio structures of selected bright Fermi blazars, based on fitting the synchrotron spectrum to VLBA images made at seven frequencies in a 4.6 -- 43.2 GHz range. Upper limits of B

Alkuperäiskieli	Englanti
Otsikko	2009 Fermi Symposium, Washington, DC, Nov 2-5; eConf Proceedings
Sivumäärä	7
Vuosikerta	C091122
Tila	Julkaistu - 2010
OKM-julkaisutyyppi	A4 Artikkeli konferenssijulkaisussa

Pääsy asiakirjaan

http://adsabs.harvard.edu/abs/2010arXiv1001.2591S

Siteeraa tätä

Sokolovsky, K. V., Kovalev, Y. Y., Lobanov, A. P., Savolainen, T., Pushkarev, A. B., & Kadler, M. (2010). Constraining the magnetic field in the parsec-scale jets of the brightest Fermi blazars with multifrequency VLBI observations. teoksessa 2009 Fermi Symposium, Washington, DC, Nov 2-5; eConf Proceedings (Vuosikerta C091122) http://adsabs.harvard.edu/abs/2010arXiv1001.2591S

@inproceedings{e60bfda8f8cc483c92fe820ea2d90770,

title = "Constraining the magnetic field in the parsec-scale jets of the brightest Fermi blazars with multifrequency VLBI observations",

abstract = "The spatially resolved broad-band spectroscopy with Very Long Baseline Interferometry (VLBI) is one of the few methods that can probe the physical conditions inside blazar jets. We report on measurements of the magnetic field strength in parsec-scale radio structures of selected bright Fermi blazars, based on fitting the synchrotron spectrum to VLBA images made at seven frequencies in a 4.6 -- 43.2 GHz range. Upper limits of B ",

keywords = "Astrophysics - Galaxy Astrophysics, Astrophysics - High Energy Astrophysical Phenomena",

author = "Sokolovsky, {K. V.} and Kovalev, {Y. Y.} and Lobanov, {A. P.} and T. Savolainen and Pushkarev, {A. B.} and M. Kadler",

year = "2010",

language = "English",

volume = "C091122",

booktitle = "2009 Fermi Symposium, Washington, DC, Nov 2-5; eConf Proceedings",

}

Constraining the magnetic field in the parsec-scale jets of the brightest Fermi blazars with multifrequency VLBI observations. / Sokolovsky, K. V.; Kovalev, Y. Y.; Lobanov, A. P. et al.
2009 Fermi Symposium, Washington, DC, Nov 2-5; eConf Proceedings. Vuosikerta C091122 2010.

Tutkimustuotos: Artikkeli kirjassa/konferenssijulkaisussa › Conference article in proceedings › Scientific › vertaisarvioitu

TY - GEN

T1 - Constraining the magnetic field in the parsec-scale jets of the brightest Fermi blazars with multifrequency VLBI observations

AU - Sokolovsky, K. V.

AU - Kovalev, Y. Y.

AU - Lobanov, A. P.

AU - Savolainen, T.

AU - Pushkarev, A. B.

AU - Kadler, M.

PY - 2010

Y1 - 2010

N2 - The spatially resolved broad-band spectroscopy with Very Long Baseline Interferometry (VLBI) is one of the few methods that can probe the physical conditions inside blazar jets. We report on measurements of the magnetic field strength in parsec-scale radio structures of selected bright Fermi blazars, based on fitting the synchrotron spectrum to VLBA images made at seven frequencies in a 4.6 -- 43.2 GHz range. Upper limits of B

AB - The spatially resolved broad-band spectroscopy with Very Long Baseline Interferometry (VLBI) is one of the few methods that can probe the physical conditions inside blazar jets. We report on measurements of the magnetic field strength in parsec-scale radio structures of selected bright Fermi blazars, based on fitting the synchrotron spectrum to VLBA images made at seven frequencies in a 4.6 -- 43.2 GHz range. Upper limits of B

KW - Astrophysics - Galaxy Astrophysics

KW - Astrophysics - High Energy Astrophysical Phenomena

M3 - Conference article in proceedings

VL - C091122

BT - 2009 Fermi Symposium, Washington, DC, Nov 2-5; eConf Proceedings

ER -

Constraining the magnetic field in the parsec-scale jets of the brightest Fermi blazars with multifrequency VLBI observations

Abstrakti

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