Hostname: page-component-77c89778f8-gq7q9 Total loading time: 0 Render date: 2024-07-18T19:49:50.711Z Has data issue: false hasContentIssue false
  • English
  • Français

3C 345: The Periods in the Optical Variability and Further Confirmation of a Connection between Optical Outbursts and Superluminal Components of Radiojet

Published online by Cambridge University Press:  19 July 2016

M.K. Babadzhanyants  and
E.T. Belokon'
M.K. Babadzhanyants
Affiliation:
Astronomical Institute of St. Petersburg University Peterhof, St. Petersburg, 198904, Russia
E.T. Belokon'
Affiliation:
Astronomical Institute of St. Petersburg University Peterhof, St. Petersburg, 198904, Russia

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present new results of our monitoring program for the superluminal quasar 3C 345 having been in continuous operation since 1968. The photographic B-band observations newly reported were made in 1984-91 during 218 nights. The optical light curve (1965-91) containing all available B-band observations was obtained.

Type
Poster Contributions: Variability
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 390
Copyright
Copyright © Kluwer 1994 

References

Babadzhanyants, M.K. and Belokon, E.T.: 1985, Astrofizika vol. 23, pp. 459–471. English translation: Astrophysics Vol. 23, pp. 639–649 Google Scholar
Barbieri, C., Romano, G., di Serego, S., Zambon, M.: 1977, A&A vol. 59, pp. 419–426 Google Scholar
Kinman, T.D., Lamia, E., Ciurla, T., Harlan, E., Wirtanen, C.A.: 1968, Ap. J. vol. 152, pp. 357–374 Google Scholar
Tang, G., Ronnang, B. and Baath, L.: 1989, A&A vol. 216, pp. 31–38 Google Scholar