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36. Commission De La Spectrophotometrie
Published online by Cambridge University Press: 25 April 2016
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By publishing at each meeting a report on the progress of astronomical spectrophotometry, our Commission has done in the past work which has been appreciated. Such a report may be expected to be of special usefulness in the present circumstances, after the disruption of normal communications for so many years. For this purpose, an attempt has been made to give a list of the most important publications, as a bibliographical appendix to this report. The titles are quoted in abridged form. My thanks are due to many members of the Commission, who contributed materially to this list and helped me with important information. I apologize for omissions, nearly inevitable in this post-war period. In future some restriction of the field of our activity ought to be considered; spectrophotometry is nowadays so general an astrophysical method, that it is nearly impossible to give a more or less complete survey of its applications to all different fields of our science. This report was finished on January 1, 1948. A few recent publications have been included in the bibliographical list.
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- Part III. Rapports et Comptes rendus
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- Copyright
- Copyright © Cambridge University Press 1950
References
page no 369 note * Figures in square brackets refer to entries in the Bibliography on pp. 385-98. The Roman numerals indicate the sections under which they are numbered.
page no 376 note * Note added in proof. Very recently a systematic analysis of the solar atmosphere by the same author was published [x, 18].
page no 376 note † Special spectrophotometry of variables, stars with extended atmospheres, etc., has not been included.
page no 398 note * Trans. I.A.U. 6, 418, 1938.
page no 399 note * The same had already been suggested by Menzel, D. H., Ap. J. 84, 465, 1936 Google Scholar.
page no 400 note * Cf.van der Held, , Zs.f. Phys. 70, 508, 1931 CrossRefGoogle Scholar; Minnaert and Slob, Proc. Acad. Amsterdam, 34, 542, 1931; Mitchell, and Zemansky, , Resonance Radiation and Excited Atoms (Cambridge, 1934)Google Scholar; Unsöld, Physik der Sternatmosphdren, pp. 168, 266, etc.
page no 400 note † This has already been done by Allen, , Mem. Commonwealth Solar Obs. 5, 21, 1934 Google Scholar.
page no 401 note * Menzel, loc. cit. p. 472.
page no 401 note † Physik der Sternatmospharen, p. 269.
page no 403 note * After the meeting, the Sub-Commission decided: the equivalent width W shall be expressed ordinarily in milli-Angstrom (mA); the reduced width A shall be expressed in Fraunhofer (F).
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