Equivalent width of OI λ7774 and absolute magnitude relation for F and G supergiants

dc.contributor.author	Kameswara Rao, N
dc.contributor.author	Mallik, S. G. V
dc.date.accessioned	2008-12-16T11:39:22Z
dc.date.available	2008-12-16T11:39:22Z
dc.date.issued	1978-04
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 183, pp. 211 - 214	en
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/2248/4071
dc.description	Open Access
dc.description.abstract	Luminosity calibration is established for F5-G2 supergiants using the equivalent width measures of OI λ7774 and FeI λ7748	en
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1978MNRAS.183..211R	en
dc.relation.uri	http://www3.interscience.wiley.com/journal/117974593/toc?func=showIssues&code=mnr
dc.rights	Royal Astronomical Society
dc.subject	F Stars	en
dc.subject	G Stars	en
dc.subject	Oxygen Spectra	en
dc.subject	Spectral Line Width	en
dc.subject	Stellar Magnitude	en
dc.subject	Supergiant Stars	en
dc.subject	Abundance	en
dc.subject	Star Clusters	en
dc.subject	Stellar Luminosity	en
dc.subject	Stellar Spectrophotometry	en
dc.title	Equivalent width of OI λ7774 and absolute magnitude relation for F and G supergiants	en
dc.type	Article	en