Measurements of Tcbr at 1. 3 MM

  • Eliana Palazzi
  • Nazzareno Mandolesi
  • Philippe Crane
  • Dennis J. Hegyi
  • J. Christopher Blades
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 155)

Abstract

The determination of TCBR at 1.3 mm is particularly interesting because it lies just at the peak of the Black-Body spectrum, where deviations can be most likely (Matsumoto et al., 1988). However, measurements at this wavelength are extremely difficult from the ground.

Keywords

Column Density Equivalent Width Local Excitation Line Equivalent Intrinsic Width 
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. Crane, P, and Hegyi, D.J., 1988, Astrophys. J.CLettersJ, L35, 326.Google Scholar
  2. Crane, P., Hegyi, D.J., Mandolesi, N., and Danks, A.C.D., 1986, Astrophys. J., 309, 822.ADSCrossRefGoogle Scholar
  3. Matsumoto, T., Hayakawa, S., Matsuo, H., Murakami, H., Sata, S., Lange, A.E., and Richards, P.L., 1988, Astrophys. J., 329, 567.ADSCrossRefGoogle Scholar

Copyright information

© Kluwer Academic Publisher 1989

Authors and Affiliations

  • Eliana Palazzi
    • 1
  • Nazzareno Mandolesi
    • 1
  • Philippe Crane
    • 2
  • Dennis J. Hegyi
    • 3
  • J. Christopher Blades
    • 4
  1. 1.Istituto TE. S. R. E. -CNRBolognaItaly
  2. 2.European Southern ObservatoryMunichDeutschland
  3. 3.University of Michigan Ann ArborUSA
  4. 4.Space Telescope Science InstituteBaItimaraUSA

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