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The maximum effect of convection in stellar atmospheres on the observed properties of stellar spectra

Przybylski, Antoni


In spite of many attempts to solve the problem of convection in stellar atmospheres our present knowledge of its effects on the structure of the outer layers of stars is still inadequate. The observations of solar granulation and theoretical investigations show clearly that there is an unstable zone in stellar atmospheres, in which the transfer of energy is partly due to radiation and partly to convection and in which therefore the actual temperature gradient has a value intermediate between...[Show more]

CollectionsOpen Access Theses
Date published: 1953
Type: Thesis (PhD)
DOI: 10.25911/5d78da67c606f


File Description SizeFormat Image
02Whole_Przybylski.pdfWhole Thesis3.65 MBAdobe PDFThumbnail
01Front_Przybylski.pdfFront Matter182.84 kBAdobe PDFThumbnail

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