Hostname: page-component-745bb68f8f-cphqk Total loading time: 0 Render date: 2025-02-03T08:58:28.121Z Has data issue: false hasContentIssue false
  • English
  • Français

4.11. 3 μm spectroscopy of galactic nuclei

Published online by Cambridge University Press:  25 May 2016

M. Imanishi ,
H. Terada ,
M. Goto  and
T. Maihara
M. Imanishi
Affiliation:
Department of Physics, Kyoto University, Kitashirakawa, Kyoto, 606-01, Japan
H. Terada
Affiliation:
Department of Physics, Kyoto University, Kitashirakawa, Kyoto, 606-01, Japan
M. Goto
Affiliation:
Department of Physics, Kyoto University, Kitashirakawa, Kyoto, 606-01, Japan
T. Maihara
Affiliation:
Department of Physics, Kyoto University, Kitashirakawa, Kyoto, 606-01, 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.

We have carried out spectroscopic observations at 3 μm, where extinction is small, of active galaxies to study the obscured emitting regions with LEWIS(Imanishi et al. 1996) mounted on the Steward Observatory 60 and 61 inch telescopes.

Type
Part II. Nuclear Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 189 - 190
Copyright
Copyright © Kluwer 1998 

References

Imanishi, et al. 1996, PASP, 108, 1129.Google Scholar
Imanishi, et al. 1997a, PASJ, 49, 69.Google Scholar
Imanishi, et al. 1997b, in preparation.Google Scholar