High-Resolution Near-Infrared Imaging of the Powerful Radio Galaxy 3C 324 at z = 1.21 with the Subaru Telescope

@article{Yamada2000HighResolutionNI,
  title={High-Resolution Near-Infrared Imaging of the Powerful Radio Galaxy 3C 324 at z = 1.21 with the Subaru Telescope},
  author={Toru Yamada and Masaru Kajisawa and Ichi Tanaka and Toshinori Maihara and Fumihide Iwamuro and Hiroshi Terada and Miwa Goto and Kentaro Motohara and Hirohisa Tanabe and Tomoyuki Taguchi and Ryuji Hata and Masanori Iye and Masatoshi Imanishi and Yoshihiro Chikada and Michitoshi Yoshida and Chris Simpson and Toshiyuki Sasaki and George Kosugi and Tomonori Usuda and Koji Omata and Katsumi Imi},
  journal={Publications of the Astronomical Society of Japan},
  year={2000},
  volume={52},
  pages={43-51}
}
We have obtained high-resolution K ′ -band images of the powerful z = 1.206 radio galaxy 3C 324 with the Subaru telescope under seeing conditions of 0 ′′ .3–0 ′′ .4. We clearly resolved the galaxy and directly compared it to the optical images obtained with the Hubble Space Telescope. The host galaxy of 3C 324 is revealed to be a moderately luminous elliptical galaxy with a smooth light profile. The effective radius of the galaxy, as determined by profile fitting, is 1.3± 0 ′′ .1 (1.2 kpc… 

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References

SHOWING 1-9 OF 9 REFERENCES

The early Universe

In the past few years one of the most exciting areas of research in physics has been the interdisciplinary field of cosmology and particle physics. The NSF's Institute for Theoretical Physics in

Physics of thermal gaseous nebulae

It sounds good when knowing the physics of thermal gaseous nebulae in this website. This is one of the books that many people looking for. In the past, many people ask about this book as their

AJ 105, 1690 HST Data Handbook, Ver3

  • AJ 105, 1690 HST Data Handbook, Ver3
  • 1993

1690 HST Data Handbook, Ver3

  • AJ
  • 1993

Proc. SPIE 3354

  • Proc. SPIE 3354
  • 1987

Amrican Institute of Physics

  • Amrican Institute of Physics