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The Calibration of Stellar Spectra Used in Measurements of the Generalized Compton Shift
Published online by Cambridge University Press: 04 August 2017
Abstract
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In the study of the changes induced by the Compton effect and Thomson scattering on the shape of spectral lines in light traversing a chromosphere or a planetary nebula it is necessary to have accurate wavelength measurements, central intensities and half widths (FWHM) of the lines. In the comparison of FWHM measures belonging to different spectra it is useful to have the intensities of the continuum at the wavelengths of the lines. The studied spectra should have a dispersion higher than 10 Å/mm and a spectral range larger than 700 Å. A short recommendation is also given about the comparison spectrum and the calibration plate.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 111: Calibration of Fundamental Stellar Quantities , 1985 , pp. 595 - 597
- Copyright
- Copyright © Reidel 1985
References
Chandrasekhar, S.
1960, Radiative Transfer, (Dover Publications Inc., New York), p. 328.Google Scholar
Crosswhite, H. M.
1958, The Spectrum of Iron I, (The Johns Hopkins University, Baltimore).Google Scholar
Schweber, S.
1966, Relativistic Quantum Field Theory, (Harper & Row, New York), p.705.Google Scholar
Trumpler, R. J. and Weaver, H. F.
1953, Statistical Astronomy, (Dover Publications Inc., New York), p.183.Google Scholar
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