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Subarcsec 10 μm Imaging of Bipolar Flow Sources

  • P. O. Lagage
  • C. Cesarski
  • R. Jouan
  • P. Masse
  • A. Tarrius
  • S. Cabrit
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 186)

Abstract

Thanks to technological developments of detector arrays, it has been possible recently to built cameras dedicated to observations in the 10 μm atmospheric window. With these cameras, it is now easy to have access to the full angular resolution capability of 3 m class telescopes: 0.7 arcsec (the diffraction limit).

Keywords

Diffraction Limit Young Star Band Filter Reference Star Atmospheric Window 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. Dent, W.: 1988, Astrophys. J. 325, 252ADSCrossRefGoogle Scholar
  2. Dent, W., Sandell, G., Duncan, W., Robson, E.: 1989, M.N.R.A.S. 238, 1497ADSGoogle Scholar
  3. Lagage, P.O.: 1989, in J.P. Swings, ed(s)., “New Technologies for Astronomy”, published by SPIE, 1130, 169Google Scholar
  4. Lagage, P.O.: 1992, in preparation Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1993

Authors and Affiliations

  • P. O. Lagage
    • 1
  • C. Cesarski
    • 1
  • R. Jouan
    • 1
  • P. Masse
    • 1
  • A. Tarrius
    • 1
  • S. Cabrit
    • 2
  1. 1.Service d’AstrophysiqueGif-Sur-YvetteFrance
  2. 2.Observatoire de GrenobleFrance

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