Skip to main content

Part of the book series: NATO ASI Series ((ASIC,volume 249))

  • 77 Accesses

Abstract

Ginga (Astro-C), the X-ray astronomy observatory of Japan, was launched on February 5, 1987. The main features and capabilities of Ginga are described. Some of the results of the observations of galactic and extragalactic sources obtained so far are presented.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 39.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 54.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1988 Kluwer Academic Publishers

About this chapter

Cite this chapter

Tanaka, Y. (1988). First Results from Ginga. In: Pallavicini, R. (eds) Hot Thin Plasmas in Astrophysics. NATO ASI Series, vol 249. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3065-0_24

Download citation

  • DOI: https://doi.org/10.1007/978-94-009-3065-0_24

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7878-8

  • Online ISBN: 978-94-009-3065-0

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics