Hostname: page-component-77c89778f8-cnmwb Total loading time: 0 Render date: 2024-07-18T08:33:11.367Z Has data issue: false hasContentIssue false
  • English
  • Français

Near-Infrared Spectroscopy of Seyfert and Starburst Galaxies

Published online by Cambridge University Press:  07 August 2017

Minoru Nishida  and
Kimiaki Kawara
Minoru Nishida
Affiliation:
Department of Physics, Kyoto University, Kyoto 606, JAPAN
Kimiaki Kawara
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo 181, JAPAN

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 Brackett α and γ lines of atomic hydrogen, molecular hydrogen H2 v=1-0 S(1) line and [FeII] 1.644 μm line were observed in type 1 and type 2 Seyferts, LINERS, starburst galaxies, and interacting galaxies. For the observations, the Infrared Spectrometer (IRS) with an array of eight InSb detectors was used on the CTIO 4 m and 1.5 m telescopes. The effective size of the slit is 6.8″x4.3″ on the 4 m and 10.3″x20.7″ on the 1.5 m. The resolution of the IRS was 290 km s−1 at 2 μm.

Type
Part 5: Structure of the Central Object and NLR
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 301 - 302
Copyright
Copyright © Kluwer 1989 

References

Kawara, K., Nishida, M., and Gregory, B. 1987, Ap. J. (Lett.) 321, L35.Google Scholar
Kawara, K., Nishida, M., and Taniguchi, Y. 1988, Ap, J.(Lett.) 328, L41.Google Scholar
Kawara, K., Nishida, M., and Phillips, M. 1989, Ap. J. Feb. 1.Google Scholar
Mouri, H., Nishida, M., Taniguchi, Y., and Kawara, K. 1988, in preparation.Google Scholar