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The connection between the parsec-scale radio jet and γ-ray flares in the blazar 1156+295. / Ramakrishnan, Venkatessh; Leon-Tavares, Jonathan; Rastorgueva-Foi, Elizaveta A.; Wiik, Kaj; Jorstad, Svetlana G.; Marscher, Alan P.; Tornikoski, Merja; Agudo, Ivan; Lahteenmaki, Anne; Valtaoja, Esko; Aller, Margo F.; Blinov, Dmitry A.; Casadio, Carolina; Efimova, Natalia V.; Gurwell, Mark A.; Gomez, Jose L.; Hagen-Thorn, Vladimir A.; Joshi, Manasvita; Jarvela, Emilia; Konstantinova, Tatiana S.; Kopatskaya, Evgenia N.; Larionov, Valeri M.; Larionova, Elena G.; Larionova, Liudmilla V.; Lavonen, Niko; MacDonald, Nicholas R.; McHardy, Ian M.; Molina, Sol N.; Morozova, Daria A.; Nieppola, Elina; Tammi, Joni; Taylor, Brian W.; Troitsky, Ivan S.

в: Monthly Notices of the Royal Astronomical Society, Том 445, № 2, 2014, стр. 1636-1646.

Результаты исследований: Научные публикации в периодических изданиях › статья

Harvard

Ramakrishnan, V, Leon-Tavares, J, Rastorgueva-Foi, EA, Wiik, K, Jorstad, SG, Marscher, AP, Tornikoski, M, Agudo, I, Lahteenmaki, A, Valtaoja, E, Aller, MF, Blinov, DA, Casadio, C, Efimova, NV, Gurwell, MA, Gomez, JL, Hagen-Thorn, VA, Joshi, M, Jarvela, E, Konstantinova, TS, Kopatskaya, EN, Larionov, VM, Larionova, EG, Larionova, LV, Lavonen, N, MacDonald, NR, McHardy, IM, Molina, SN, Morozova, DA, Nieppola, E, Tammi, J, Taylor, BW & Troitsky, IS 2014, 'The connection between the parsec-scale radio jet and γ-ray flares in the blazar 1156+295', Monthly Notices of the Royal Astronomical Society, Том. 445, № 2, стр. 1636-1646. https://doi.org/10.1093/mnras/stu1873

APA

Ramakrishnan, V., Leon-Tavares, J., Rastorgueva-Foi, E. A., Wiik, K., Jorstad, S. G., Marscher, A. P., Tornikoski, M., Agudo, I., Lahteenmaki, A., Valtaoja, E., Aller, M. F., Blinov, D. A., Casadio, C., Efimova, N. V., Gurwell, M. A., Gomez, J. L., Hagen-Thorn, V. A., Joshi, M., Jarvela, E., ... Troitsky, I. S. (2014). The connection between the parsec-scale radio jet and γ-ray flares in the blazar 1156+295. Monthly Notices of the Royal Astronomical Society, 445(2), 1636-1646. https://doi.org/10.1093/mnras/stu1873

Vancouver

Ramakrishnan V, Leon-Tavares J, Rastorgueva-Foi EA, Wiik K, Jorstad SG, Marscher AP и пр. The connection between the parsec-scale radio jet and γ-ray flares in the blazar 1156+295. Monthly Notices of the Royal Astronomical Society. 2014;445(2):1636-1646. https://doi.org/10.1093/mnras/stu1873

Author

Ramakrishnan, Venkatessh ; Leon-Tavares, Jonathan ; Rastorgueva-Foi, Elizaveta A. ; Wiik, Kaj ; Jorstad, Svetlana G. ; Marscher, Alan P. ; Tornikoski, Merja ; Agudo, Ivan ; Lahteenmaki, Anne ; Valtaoja, Esko ; Aller, Margo F. ; Blinov, Dmitry A. ; Casadio, Carolina ; Efimova, Natalia V. ; Gurwell, Mark A. ; Gomez, Jose L. ; Hagen-Thorn, Vladimir A. ; Joshi, Manasvita ; Jarvela, Emilia ; Konstantinova, Tatiana S. ; Kopatskaya, Evgenia N. ; Larionov, Valeri M. ; Larionova, Elena G. ; Larionova, Liudmilla V. ; Lavonen, Niko ; MacDonald, Nicholas R. ; McHardy, Ian M. ; Molina, Sol N. ; Morozova, Daria A. ; Nieppola, Elina ; Tammi, Joni ; Taylor, Brian W. ; Troitsky, Ivan S. / The connection between the parsec-scale radio jet and γ-ray flares in the blazar 1156+295. в: Monthly Notices of the Royal Astronomical Society. 2014 ; Том 445, № 2. стр. 1636-1646.

BibTeX

@article{a829361e86ca48978e62e499d55a2acb,
title = "The connection between the parsec-scale radio jet and γ-ray flares in the blazar 1156+295",
abstract = "{\textcopyright} 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. The blazar 1156+295 was active at γ-ray energies, exhibiting three prominent flares during the year 2010. Here, we present results using the combination of broad-band (X-ray through mm single-dish) monitoring data and radio-band imaging data at 43 GHz on the connection of γ-ray events to the ejections of superluminal components and other changes in the jet of 1156+295. The kinematics of the jet over the interval 2007.0-2012.5 using 43 GHz Very Long Baseline Array observations reveal the presence of four moving and one stationary component in the inner region of the blazar jet. The propagation of the third and fourth components in the jet corresponds closely in time to the active phase of the source in γ-rays. We briefly discuss the implications of the structural changes in the jet for the mechanism of γ-ray production during bright flares. To localize the γ-ray emission site in the blazar, we performed the cor",
author = "Venkatessh Ramakrishnan and Jonathan Leon-Tavares and Rastorgueva-Foi, {Elizaveta A.} and Kaj Wiik and Jorstad, {Svetlana G.} and Marscher, {Alan P.} and Merja Tornikoski and Ivan Agudo and Anne Lahteenmaki and Esko Valtaoja and Aller, {Margo F.} and Blinov, {Dmitry A.} and Carolina Casadio and Efimova, {Natalia V.} and Gurwell, {Mark A.} and Gomez, {Jose L.} and Hagen-Thorn, {Vladimir A.} and Manasvita Joshi and Emilia Jarvela and Konstantinova, {Tatiana S.} and Kopatskaya, {Evgenia N.} and Larionov, {Valeri M.} and Larionova, {Elena G.} and Larionova, {Liudmilla V.} and Niko Lavonen and MacDonald, {Nicholas R.} and McHardy, {Ian M.} and Molina, {Sol N.} and Morozova, {Daria A.} and Elina Nieppola and Joni Tammi and Taylor, {Brian W.} and Troitsky, {Ivan S.}",
year = "2014",
doi = "10.1093/mnras/stu1873",
language = "English",
volume = "445",
pages = "1636--1646",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Wiley-Blackwell",
number = "2",

}

RIS

TY - JOUR

T1 - The connection between the parsec-scale radio jet and γ-ray flares in the blazar 1156+295

AU - Ramakrishnan, Venkatessh

AU - Leon-Tavares, Jonathan

AU - Rastorgueva-Foi, Elizaveta A.

AU - Wiik, Kaj

AU - Jorstad, Svetlana G.

AU - Marscher, Alan P.

AU - Tornikoski, Merja

AU - Agudo, Ivan

AU - Lahteenmaki, Anne

AU - Valtaoja, Esko

AU - Aller, Margo F.

AU - Blinov, Dmitry A.

AU - Casadio, Carolina

AU - Efimova, Natalia V.

AU - Gurwell, Mark A.

AU - Gomez, Jose L.

AU - Hagen-Thorn, Vladimir A.

AU - Joshi, Manasvita

AU - Jarvela, Emilia

AU - Konstantinova, Tatiana S.

AU - Kopatskaya, Evgenia N.

AU - Larionov, Valeri M.

AU - Larionova, Elena G.

AU - Larionova, Liudmilla V.

AU - Lavonen, Niko

AU - MacDonald, Nicholas R.

AU - McHardy, Ian M.

AU - Molina, Sol N.

AU - Morozova, Daria A.

AU - Nieppola, Elina

AU - Tammi, Joni

AU - Taylor, Brian W.

AU - Troitsky, Ivan S.

PY - 2014

Y1 - 2014

N2 - © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. The blazar 1156+295 was active at γ-ray energies, exhibiting three prominent flares during the year 2010. Here, we present results using the combination of broad-band (X-ray through mm single-dish) monitoring data and radio-band imaging data at 43 GHz on the connection of γ-ray events to the ejections of superluminal components and other changes in the jet of 1156+295. The kinematics of the jet over the interval 2007.0-2012.5 using 43 GHz Very Long Baseline Array observations reveal the presence of four moving and one stationary component in the inner region of the blazar jet. The propagation of the third and fourth components in the jet corresponds closely in time to the active phase of the source in γ-rays. We briefly discuss the implications of the structural changes in the jet for the mechanism of γ-ray production during bright flares. To localize the γ-ray emission site in the blazar, we performed the cor

AB - © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. The blazar 1156+295 was active at γ-ray energies, exhibiting three prominent flares during the year 2010. Here, we present results using the combination of broad-band (X-ray through mm single-dish) monitoring data and radio-band imaging data at 43 GHz on the connection of γ-ray events to the ejections of superluminal components and other changes in the jet of 1156+295. The kinematics of the jet over the interval 2007.0-2012.5 using 43 GHz Very Long Baseline Array observations reveal the presence of four moving and one stationary component in the inner region of the blazar jet. The propagation of the third and fourth components in the jet corresponds closely in time to the active phase of the source in γ-rays. We briefly discuss the implications of the structural changes in the jet for the mechanism of γ-ray production during bright flares. To localize the γ-ray emission site in the blazar, we performed the cor

U2 - 10.1093/mnras/stu1873

DO - 10.1093/mnras/stu1873

M3 - Article

VL - 445

SP - 1636

EP - 1646

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -

ID: 7033359