Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T08:34:12.666Z Has data issue: false hasContentIssue false
  • English
  • Français

New AGNs Discovered with the 2.16-m Telescope at Xinglong Station of Beijing Astronomical Observatory1

Published online by Cambridge University Press:  12 April 2016

Z. L. Zou  and
Q. B. Li
Z. L. Zou
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Q. B. Li
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, 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.

The preliminary results of several on-going AGN programs using the 2.16-m telescope at Xinglong Station of Beijing Astronomical Observatory are described. About 150 new AGNs including QSOs, BL Lac objects, and Seyferts have been discovered in the last two years.

Type
IX. Surveys and Properties of Active Galaxies and Related Sources
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 413 - 418
Copyright
Copyright © Astronomical Society of the Pacific 1997

Footnotes

1

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

References

Allen, D.A., Norris, R.P., Meadows, V.S., & Roche, P.F. 1991, MNRAS, 248, 528.Google Scholar
Brinkmann, W., et al. 1995, A&AS, 109, 147.Google Scholar
Chen, J.S. 1995, Astrophysics Reports, Publ. BAO, No. 26, 1.Google Scholar
De Grijp, M.H., Miley, G.K., Lub, J., & de Jong, T. 1985, Nature, 314, 240.CrossRefGoogle Scholar
Gu, Q.S., Huang, J.H., Shang, Z.H., Su, H.J., & Zhu, J. 1995, ApSS, 229, 317.Google Scholar
He, R., & Chen, J.S. 1993, ApSS, 200, 279.Google Scholar
He, X.T. & Impey, C.D. 1986, MNRAS, 221, 727.CrossRefGoogle Scholar
Huang, J.H., Gu, Q.S., Su, H.J., & Shang, Z.H. 1996a, A&A, 311, 21.Google Scholar
Huang, J.H., Gu, Q.S., Su, H.J., & Shang, Z.H. 1996b, ApSS, 235, 109.Google Scholar
Huang, K.L., & Huang, J.H. 1986, ApSS, 125, 85.Google Scholar
Strauss, M.A., et al. 1992, ApJS, 83, 29.Google Scholar
Veilleux, S., & Osterbrock, D.E. 1987, ApJS, 63, 295.CrossRefGoogle Scholar
Véron-Cetty, M.-P., & Véron, P. 1993, ESO Scientific Report No. 13.Google Scholar
Wei, J.Y., Wu, X.B., Hu, J.Y., & Li, Q.B. 1995, Acta Astrophysica Sinica, 15, 390.Google Scholar
Wei, J.Y, Cao, L., Hu, J.Y., & Li, Q.B. 1997, this volume.Google Scholar
Wu, H. 1996, Ph.D. thesis, Beijing Astronomical Observatory.Google Scholar
Wu, H., Zou, Z.L., Xia, X.Y., & Deng, Z.G. 1997, this volume.Google Scholar
Wu, H., Zou, Z.L., & Chen, J.S. 1995, Acta Astronomica Sinica, 36, 428.Google Scholar
Wu, X.B. 1996, Ph.D. thesis, Beijing Astronomical Observatory.Google Scholar
Zhan, Y., & Chen, J.S. 1989, Acta Astrophysica Sinica, 9, 37.Google Scholar
Zhao, Y.H., Zhong, J.X., Li, Q.B., & Hu, J.Y. 1994, Acta Astrophysica Sinica, 14, 385.Google Scholar
Zhao, Y.H., Zhong, J.X., Hu, J.Y., & Li, Q.B. 1997, this volume.Google Scholar
Zou, Z.L., Xia, X.Y., Deng, Z.G., & Wu, H. 1995, A&A, 304, 369.Google Scholar