Hostname: page-component-77c89778f8-7drxs Total loading time: 0 Render date: 2024-07-18T22:24:17.404Z Has data issue: false hasContentIssue false
  • English
  • Français

Optical Monitoring of 3C 390.3 in 19951

Published online by Cambridge University Press:  12 April 2016

Bo-Chen Qian  and
Jun Tao
Bo-Chen Qian
Affiliation:
Shanghai Observatory, The Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
Jun Tao
Affiliation:
Shanghai Observatory, The Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China

Abstract

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 light curves obtained during a seven-month monitoring campaign on 3C 390.3. The source steadily increased by about 0.5 mag from 1995 July to October.

Type
III. Broad-Line Profiles and Variability
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 165 - 166
Copyright
Copyright © Astronomical Society of the Pacific 1997

Footnotes

1

This work is supported by the National Natural Science Foundation of China.

References

Penston, M.J., Penston, M.V., & Sandage, A.R. 1971, PASP, 83, 783.Google Scholar