A precessing and nutating jet in OJ287

  • Silke Britzen
  • , C. Fendt
  • , G. Witzel
  • , S. J. Qian
  • , I. N. Pashchenko
  • , O. Kurtanidze
  • , M. Zajacek
  • , G. Martinez
  • , V. Karas
  • , M. Aller
  • , H. Aller
  • , A. Eckart
  • , K. Nilsson
  • , P. Arévalo
  • , J. Cuadra
  • , M. Subroweit
  • , A. Witzel

Producción científica: Contribución a una revistaArtículo de la conferenciarevisión exhaustiva

1 Cita (Scopus)

Resumen

We re-analyzed OJ287 in 120 Very Long Baseline Array (VLBA, MOJAVE) observations (at 15 GHz) covering the time span between Apr. 1995 and Apr. 2017. We find that the radio jet motion over the sky is consistent with a precessing and nutating jet source. The variability of the radio flux-density can be explained by Doppler beaming due to a change in the viewing angle. We suggest that part of the optical emission is due to synchrotron emission related to the jet radiation. We find a strikingly similar scaling for the timescales for precession and nutation as indicated for SS433 with a factor of roughly 50 times longer in OJ287.

Idioma originalInglés
Páginas (desde-hasta)250-251
Número de páginas2
PublicaciónProceedings of the International Astronomical Union
Volumen14
N.º342
DOI
EstadoPublicada - 2020
Publicado de forma externa
Evento342nd Symposium of the International Astronomical on Perseus in Sicily: From Black Hole to Cluster Outskirts - Noto, Italia
Duración: 14 may. 201818 may. 2018

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