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The jet in the radio galaxy 3C120 : Jet/cloud interactions at parsec scales. / Gómez, J. L.; Marscher, A. P.; Jorstad, S. G.; Agudo, I.

в: Astronomische Nachrichten, Том 327, № 2-3, 2006, стр. 223-226.

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

Harvard

Gómez, JL, Marscher, AP, Jorstad, SG & Agudo, I 2006, 'The jet in the radio galaxy 3C120: Jet/cloud interactions at parsec scales', Astronomische Nachrichten, Том. 327, № 2-3, стр. 223-226. https://doi.org/10.1002/asna.200510511

APA

Gómez, J. L., Marscher, A. P., Jorstad, S. G., & Agudo, I. (2006). The jet in the radio galaxy 3C120: Jet/cloud interactions at parsec scales. Astronomische Nachrichten, 327(2-3), 223-226. https://doi.org/10.1002/asna.200510511

Vancouver

Gómez JL, Marscher AP, Jorstad SG, Agudo I. The jet in the radio galaxy 3C120: Jet/cloud interactions at parsec scales. Astronomische Nachrichten. 2006;327(2-3):223-226. https://doi.org/10.1002/asna.200510511

Author

Gómez, J. L. ; Marscher, A. P. ; Jorstad, S. G. ; Agudo, I. / The jet in the radio galaxy 3C120 : Jet/cloud interactions at parsec scales. в: Astronomische Nachrichten. 2006 ; Том 327, № 2-3. стр. 223-226.

BibTeX

@article{c0cb549d4e98494ba920448d245e790c,
title = "The jet in the radio galaxy 3C120: Jet/cloud interactions at parsec scales",
abstract = "The radio galaxy 3C 120 appears as one of the best sources to study the emission and propagation of relativistic jets in active galactic nuclei. Muti-wavelength multi-epoch observations suggest that this Seyfert 1 galaxy is probably the result of a merger and presents a jet in precession that originates from the accretion of material onto a super massive central black hole. Thanks to its proximity and high activity it is possible to monitor the rapid changing rich inner jet structure with unprecedented spatial and temporal resolutions through very long baseline interferometry observations. The jet is pointing close to the line of sight, and is most probably interacting very dynamically with a cloud of properties intermediate of those of the broad and narrow emission-line regions.",
keywords = "Galaxies: active, Galaxies: individual (3C 120), Galaxies: jets",
author = "G{\'o}mez, {J. L.} and Marscher, {A. P.} and Jorstad, {S. G.} and I. Agudo",
year = "2006",
doi = "10.1002/asna.200510511",
language = "English",
volume = "327",
pages = "223--226",
journal = "Astronomische Nachrichten",
issn = "0004-6337",
publisher = "Wiley-Blackwell",
number = "2-3",

}

RIS

TY - JOUR

T1 - The jet in the radio galaxy 3C120

T2 - Jet/cloud interactions at parsec scales

AU - Gómez, J. L.

AU - Marscher, A. P.

AU - Jorstad, S. G.

AU - Agudo, I.

PY - 2006

Y1 - 2006

N2 - The radio galaxy 3C 120 appears as one of the best sources to study the emission and propagation of relativistic jets in active galactic nuclei. Muti-wavelength multi-epoch observations suggest that this Seyfert 1 galaxy is probably the result of a merger and presents a jet in precession that originates from the accretion of material onto a super massive central black hole. Thanks to its proximity and high activity it is possible to monitor the rapid changing rich inner jet structure with unprecedented spatial and temporal resolutions through very long baseline interferometry observations. The jet is pointing close to the line of sight, and is most probably interacting very dynamically with a cloud of properties intermediate of those of the broad and narrow emission-line regions.

AB - The radio galaxy 3C 120 appears as one of the best sources to study the emission and propagation of relativistic jets in active galactic nuclei. Muti-wavelength multi-epoch observations suggest that this Seyfert 1 galaxy is probably the result of a merger and presents a jet in precession that originates from the accretion of material onto a super massive central black hole. Thanks to its proximity and high activity it is possible to monitor the rapid changing rich inner jet structure with unprecedented spatial and temporal resolutions through very long baseline interferometry observations. The jet is pointing close to the line of sight, and is most probably interacting very dynamically with a cloud of properties intermediate of those of the broad and narrow emission-line regions.

KW - Galaxies: active

KW - Galaxies: individual (3C 120)

KW - Galaxies: jets

UR - http://www.scopus.com/inward/record.url?scp=33645322390&partnerID=8YFLogxK

U2 - 10.1002/asna.200510511

DO - 10.1002/asna.200510511

M3 - Article

AN - SCOPUS:33645322390

VL - 327

SP - 223

EP - 226

JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

SN - 0004-6337

IS - 2-3

ER -

ID: 88372820