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Physical conditions in wolf-rayet atmospheres

Show simple item record Bappu, M. K. Vainu 2015-08-14T07:12:31Z 2015-08-14T07:12:31Z 1957-10-31
dc.description.abstract A critical discussion of present-day knowledge regarding the Wolf-Rayet atmosphere is presented. It is shown that the large widths usually ascribed to the emission lines are formed by heavy blending, and that the individual components are in many cases seen distinctly on high dispersion coude spectra. Arguments are given to show that the single stars alone do not yield observational information of the exact dynamical conditionals in the atmosphere. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries bnisi9-155
dc.subject Atmospheres en_US
dc.subject Wolf-rayet en_US
dc.title Physical conditions in wolf-rayet atmospheres en_US
dc.type Article en_US

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