Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-30T06:33:43.008Z Has data issue: false hasContentIssue false
  • English
  • Français

Tridimensional spectroscopy of Seyfert Galaxy 3C 120

Published online by Cambridge University Press:  12 April 2016

G. Kosugi ,
H. Ohtani ,
M. Yoshida  and
K. Aoki
G. Kosugi
Affiliation:
Department of Astronomy, Faculty of Science, Kyoto University, Kyoto 606-01
H. Ohtani
Affiliation:
Department of Astronomy, Faculty of Science, Kyoto University, Kyoto 606-01
M. Yoshida
Affiliation:
Department of Astronomy, Faculty of Science, Kyoto University, Kyoto 606-01
K. Aoki
Affiliation:
Department of Astronomy, Faculty of Science, Kyoto University, Kyoto 606-01

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.

Tridimensional spectroscopy of the Seyfert 1 galaxy 3C 120 was carried out with Spectronebulagraph (SNG). We constructed a data cube which is free from atmospheric variations during the scans. We then separated the blended lines by deconvolving the line profiles, to obtain pure narrow-line images and narrow-line intensity ratio diagram.

Type
3. Integral Field Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 205 - 206
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Ferland, G.J. 1991, OSU Internal Report 91-01Google Scholar
Kosugi, G., Ohtani, H., Sasaki, T., Shimizu, Y., Koyano, H., Yoshida, M., Baba, A., Aoki, K., & Sasaki, M. 1994a, in preparationGoogle Scholar
Kosugi, G., Ohtani, H., Yoshida, A., & Aoki, K. 1994b, in preparationGoogle Scholar
Veilleux, S., & Osterbrock, D.E. 1987, ApJS, 63, 295 Google Scholar