On the infrared bands of a A10 related to Mira phenomena

dc.contributor.author	Murty, P. S
dc.date.accessioned	2008-12-15T15:13:03Z
dc.date.available	2008-12-15T15:13:03Z
dc.date.issued	1978-04
dc.identifier.citation	Astrophysics and Space Science, Vol. 54, No. 2, pp. 509 - 512	en
dc.identifier.issn	0004-640X (Print) 1572-946X (Online)
dc.identifier.uri	http://hdl.handle.net/2248/4063
dc.description	Open Access
dc.description.abstract	The calculated band positions and intensity factors for the bands of the infrared A-X transition of A10 suggest that an investigation for the infrared bands in the 1 to 5 micron region of the spectra of Mira stars and M supergiants, along with the 'blue-green' (B-X) bands, could provide clues to the Mira phenomena. The need for additional laboratory investigation of the infrared electronic transition is emphasized	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Company	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1978Ap%26SS..54..509M	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00639453	en
dc.rights	D. Reidel Publishing Company
dc.subject	Aluminum Oxides	en
dc.subject	Infrared Spectra	en
dc.subject	Mira Variables	en
dc.subject	Stellar Spectrophotometry	en
dc.subject	Variable Stars	en
dc.subject	Line Spectra	en
dc.subject	M Stars	en
dc.subject	Supergiant Stars	en
dc.subject	Tables (Data)	en
dc.title	On the infrared bands of a A10 related to Mira phenomena	en
dc.type	Article	en