Abstract
MR. W. M. H. GREAVES1 has made certain objections to my tentative explanation of secondary maxima in the continuous spectra of novæ, etc.2, because the observations of Nova Herculis 1934 made by various observers do not fully agree.
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W. M. H. Greaves, NATURE, 137, 405 (1936).
W. M. Cohn, NATURE, 137, 150 (1936).
F. Beileke and O. Hachenberg, Z. Astrophys., 10, 366 (1935).
D. Barbier, D. Chalonge and E. Vasy, C. R., 201, 128 (1935).
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COHN, W. Continuous Spectra of Certain Types of Stars and Nebulæ. Nature 138, 127 (1936). https://doi.org/10.1038/138127a0
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DOI: https://doi.org/10.1038/138127a0
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