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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4063
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dc.contributor.authorMurty, P. S-
dc.date.accessioned2008-12-15T15:13:03Z-
dc.date.available2008-12-15T15:13:03Z-
dc.date.issued1978-04-
dc.identifier.citationAstrophysics and Space Science, Vol. 54, No. 2, pp. 509 - 512en
dc.identifier.issn0004-640X (Print) 1572-946X (Online)-
dc.identifier.urihttp://hdl.handle.net/2248/4063-
dc.descriptionOpen Access-
dc.description.abstractThe 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 emphasizeden
dc.language.isoenen
dc.publisherD. Reidel Publishing Companyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1978Ap%26SS..54..509Men
dc.relation.urihttp://dx.doi.org/10.1007/BF00639453en
dc.rightsD. Reidel Publishing Company-
dc.subjectAluminum Oxidesen
dc.subjectInfrared Spectraen
dc.subjectMira Variablesen
dc.subjectStellar Spectrophotometryen
dc.subjectVariable Starsen
dc.subjectLine Spectraen
dc.subjectM Starsen
dc.subjectSupergiant Starsen
dc.subjectTables (Data)en
dc.titleOn the infrared bands of a A10 related to Mira phenomenaen
dc.typeArticleen
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