Presence of Mg II emission in R Coronae Borealis at maximum light

Kameswara Rao, N; Nandy, K; Bappu, M. K. V

dc.contributor.author	Kameswara Rao, N
dc.contributor.author	Nandy, K
dc.contributor.author	Bappu, M. K. V
dc.date.accessioned	2007-12-01T09:54:09Z
dc.date.available	2007-12-01T09:54:09Z
dc.date.issued	1981-06
dc.identifier.citation	Monthly Notices of Royal Astronomical Society, Vol. 195, June, pp. 71-74	en
dc.identifier.uri	http://hdl.handle.net/2248/2002
dc.description.abstract	The high dipersion spectrum of R CrB in the long wavelength obtained near its maximum with the International Ultraviolet Explorer shows the presence of chromospheric Mg II emission. For comparison the spectrum of Gamma Cyg was obtained immediately afterwards. The Mg II emission width of R CrB is found to be the same as that of Gamma Cyg.	en
dc.format.extent	400783 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1981MNRAS.195P..71R	en
dc.subject	Dispersion Spectrum	en
dc.subject	Mg II Emission	en
dc.subject	Spectra	en
dc.subject	M.K.V. Bappu	en
dc.title	Presence of Mg II emission in R Coronae Borealis at maximum light	en
dc.type	Article	en