Physical conditions in wolf-rayet atmospheres

dc.contributor.author	Bappu, M. K. Vainu
dc.date.accessioned	2015-08-14T07:12:31Z
dc.date.available	2015-08-14T07:12:31Z
dc.date.issued	1957-10-31
dc.identifier.uri	http://hdl.handle.net/123456789/1197
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