Radio continuum spectra

  • M. J. Seaton
Part IV: Evolved H II regions and 0B-stars
Part of the Lecture Notes in Physics book series (LNP, volume 42)


Radio continuum flux spectra S, depend on electron temperatures Te and on angular areas Ω (E) which enclose contours of constant emission measure E. Different methods of analyzing observations are discussed.


Electron Temperature Thermal Emission Angular Resolution Emission Measure Ionize Hydrogen 
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.


Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.


  1. Bracewell, R.N. 1969, “Paris Symposium on Radio Astronomy”, Stanford Univ. Press.Google Scholar
  2. Brocklehurst, M., and Seaton, M.J. 1972, Mon. Not. R. astr. Soc., 157, 179.Google Scholar
  3. Harris, S. 1973, Mon. Not. R. astr. Soc., 162, 5P.Google Scholar
  4. Hjellming, R.M., Andrews, M.H., and Sejnowski, T.J. 1969, Ap.J., 157, 573.Google Scholar
  5. Martin, A.H.M. 1973, Mon. Not. R. astr. Soc., 163,141.Google Scholar
  6. Mezger, P.G. 1968, “Interstellar ionized hydrogen” (ed. Y. Terzian), p.459, Benjamin, New York.Google Scholar
  7. Mezger, P.G., Schraml, J., and Terzian, Y. 1967, Ap. J., 150, 807.Google Scholar
  8. Ryle, M., and Downes, D. 1967, Ap.J., 148, L.17.Google Scholar
  9. Salem, M., and Seaton,M.J. 1974, Mon. Not. R. astr. Soc., 167, 493.Google Scholar
  10. Seaton, M.J. 1974, Quart. J., R. astr. Soc., 15, 370.Google Scholar
  11. Wade, C.M. 1958, Aust.J.Phys., 11, 388. *** DIRECT SUPPORT *** A3418034 00007Google Scholar

Copyright information

© Springer-Verlag 1975

Authors and Affiliations

  • M. J. Seaton
    • 1
  1. 1.Department of Physics & AstronomyUniversity College LondonLondon WClE 6BTEngland

Personalised recommendations