Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-11T14:19:07.048Z Has data issue: false hasContentIssue false
  • English
  • Français

Variability of NGC 3783: First Results from an Intensive Ground-Based Monitoring Campaign

Published online by Cambridge University Press:  19 July 2016

Giovanna M. Stirpe
Giovanna M. Stirpe*
Affiliation:
Osservatorio Astronomico di Bologna, Via Zamboni 33, 40126 Bologna, Italy

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.

The International AGN Watch collaboration undertook an intensive monitoring campaign of the bright Seyfert 1 galaxy NGC 3783 between December 1991 and August 1992, in order to study the variations of the continuum and broad emission lines. Spectroscopic and photometric observations took place at several ground-based observatories and formed the optical/IR counterpart to the UV observations conducted with the IUE (Reichert et al. 1993).

Type
Poster Contributions: Variability
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 407
Copyright
Copyright © Kluwer 1994 

References

Reichert, G.A., et al. 1993, ApJ, in press Google Scholar
Stirpe, G.M., et al. 1993, ApJ, submitted Google Scholar