Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-26T12:13:36.548Z Has data issue: false hasContentIssue false
  • English
  • Français

Near-infrared studies of the Milky Way

Published online by Cambridge University Press:  04 August 2017

H. Okuda
H. Okuda*
Affiliation:
Institute for Space and Astronautical Science Komaba 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.

The inner region of the Galaxy has been explored by means of near-infrared observations; the distribution and population of the stars are studied from the near-infrared brightness mapping and star counts in the Milky Way, while the magnetic-field configuration is probed by the near-infrared polarimetry.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 123 - 126
Copyright
Copyright © Reidel 1985 

References

Hayakawa, S., Ito, K., Matsumoto, T., and Uyama, K.: 1977, Astron. Astrophys. 58, 325 Google Scholar
Hayakawa, S., Matsumoto, T., Murakami, H., Uyama, K., Thomas, J.A., and Yamagami, T.: 1981, Astron. Astrophys. 100, 106 Google Scholar
Kawara, K., Kozasa, T., Sato, S., Kobayashi, Y., and Okuda, H.: 1982, Pub. Astron. Soc. Japan 34, 389 Google Scholar
Maihara, T., Oda, N., Sugiyama, T., and Okuda, H.: 1978, Publ. Astron. Soc. Japan 30, 1 Google Scholar
Okuda, H.: 1981, in “Infrared Astronomy”, IAU Symp. No. 96, review p. 247.Google Scholar