Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-26T03:34:23.197Z Has data issue: false hasContentIssue false
  • English
  • Français

Wide-Field Imaging of Nearby Galaxies in Near-Infrared Bands

Published online by Cambridge University Press:  26 July 2016

T. Ichikawa ,
K. Tarusawa ,
K. Yanagisawa ,
N. Itoh  and
M. Ueno
T. Ichikawa
Affiliation:
Kiso Observatory, University of Tokyo, Mitake-Mura, Kiso-gun, Nagano 397-01, Japan
K. Tarusawa
Affiliation:
Kiso Observatory, University of Tokyo, Mitake-Mura, Kiso-gun, Nagano 397-01, Japan
K. Yanagisawa
Affiliation:
Department of Astronomy, University of Tokyo, Yayoi, Bunkyo-ku, Tokyo 113, Japan
N. Itoh
Affiliation:
Department of Astronomy, University of Tokyo, Yayoi, Bunkyo-ku, Tokyo 113, Japan
M. Ueno
Affiliation:
College of Arts and Science, University of Tokyo, Komaba, Meguro-ku, Tokyo 153, Japan

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.

We present the results of wide-field imaging of nearby galaxies observed in the near-infrared using a large format array. The total magnitudes and mass-to-luminosity ratios of NGC 253, M 82, NGC 891, and some cluster members are discussed.

Type
Part Twelve: Properties of Nearby Galaxies
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 599 - 600
Copyright
Copyright © Kluwer 1994 

References

Haynes, and Giovanelli, , 1984. Astron. J., 89, 758.CrossRefGoogle Scholar
Sofue, et al., 1992. Astrophys. J., 395, 126.CrossRefGoogle Scholar
Ueno, et al., 1992. S.P.I.E., 1762, 423.Google Scholar