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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4071
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dc.contributor.authorKameswara Rao, N-
dc.contributor.authorMallik, S. G. V-
dc.date.accessioned2008-12-16T11:39:22Z-
dc.date.available2008-12-16T11:39:22Z-
dc.date.issued1978-04-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 183, pp. 211 - 214en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/4071-
dc.descriptionOpen Access-
dc.description.abstractLuminosity calibration is established for F5-G2 supergiants using the equivalent width measures of OI λ7774 and FeI λ7748en
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1978MNRAS.183..211Ren
dc.relation.urihttp://www3.interscience.wiley.com/journal/117974593/toc?func=showIssues&code=mnr-
dc.rightsRoyal Astronomical Society-
dc.subjectF Starsen
dc.subjectG Starsen
dc.subjectOxygen Spectraen
dc.subjectSpectral Line Widthen
dc.subjectStellar Magnitudeen
dc.subjectSupergiant Starsen
dc.subjectAbundanceen
dc.subjectStar Clustersen
dc.subjectStellar Luminosityen
dc.subjectStellar Spectrophotometryen
dc.titleEquivalent width of OI λ7774 and absolute magnitude relation for F and G supergiantsen
dc.typeArticleen
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