Skip to main content

Galactic Structure from the Two Micron Galactic Survey

  • Conference paper
  • 56 Accesses

Abstract

The Two Micron Galactic Survey (TMGS) is the most sensitive large scale point source near infrared survey of the Galactic Plane yet attempted. The Galactic plane has been drift-scanned in several regions over the areas -5° < l < 30°, |b|≤ 15° and 30° < l < 180°, |b|≤ 5°.The survey is complete in the areas covered to magnitude m k = +9.8. So far, a total area of 255 square degrees has been mapped and 500000 objects have been detected, the majority of these in the Galactic plane and with no visible counterparts. In this contribution we use data from the TMGS to probe the star distribution within the Galactic disk.

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

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   129.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD   169.99
Price excludes VAT (USA)
  • Durable hardcover 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

Learn about institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  • Garzón F., Hammersley P., Mahoney T., Calbet X., Selby M. J., Hepburn I., 1993 MNRAS, 264, 773

    ADS  Google Scholar 

  • Hayakawa S., Ito K., Matsumoto T., Murakami H., Uyama K., 1978, PASJ, 30, 369

    ADS  Google Scholar 

  • Ito K., Matsumoto T., Uyama K., 1976, PASJ, 28, 427

    ADS  Google Scholar 

  • Ito K., Matsumoto T., Uyama K., 1977, Nat, 265, 517

    Article  ADS  Google Scholar 

  • Maihara T., Oda N., Sugiyama T., Okuda H., 1978, PASJ, 30, 1

    ADS  Google Scholar 

  • Melnick G. J., Fazio G. G., Koch D. G., Rieke G. H., Young E. T., Low F. J., Hoffmann W. F., Gautier T. N., 1987, in Backer D. C., ed., Proc. symp. honoring C. H. Townes, The Galactic Center, Berkeley CA, 1986. AIP, New York

    Google Scholar 

  • Schmidt-Kaler T., 1976, Vistas Astron., 19, 69

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1994 Springer Science+Business Media Dordrecht

About this paper

Cite this paper

Garzón, F., Hammersley, P.L., Mahoney, T., Calbet, X., Selby, M.J. (1994). Galactic Structure from the Two Micron Galactic Survey. In: Epchtein, N., Omont, A., Burton, B., Persi, P. (eds) Science with Astronomical Near-Infrared Sky Surveys. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0946-8_39

Download citation

  • DOI: https://doi.org/10.1007/978-94-011-0946-8_39

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4408-0

  • Online ISBN: 978-94-011-0946-8

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics