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DENIS and ISOCAM Observations of Chamaeleon I Cloud

  • P. Persi
  • E. Copet
  • A. A. Kaas
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 230)

Abstract

We present the results of the observations of the Chamaeleon I molecular cloud, in DENIS near-infrared (I, J and K s ) and ISOCAM mid-infrared (LW2, LW3).

Keywords

Molecular Cloud Luminosity Function Spectral Energy Distribution Tauri Star Circumstellar Disk 
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.

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References

  1. Cambrésy L., Epchtein N., Copet E., De Batz B., Kimeswenger S., Le Bertre T., Rouan D. and Tiphène D. (1997) A&A, 324, p.L5ADSGoogle Scholar
  2. Cesarsky C (+ 20 authors) (1996) A&A, 315L, p. 32ADSGoogle Scholar
  3. Nordh L (+20 authors) (1996) A&A, 315L, p. 185ADSGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1998

Authors and Affiliations

  • P. Persi
    • 1
  • E. Copet
    • 2
  • A. A. Kaas
    • 3
  1. 1.Istituto Astrofisica SpazialeCNRFrascatiItaly
  2. 2.Observatoire de ParisDESPAMeudon CedexFrance
  3. 3.Stockolm ObservatorySaltsjöbadenSwenden

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