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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4565
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dc.contributor.authorParthasarathy, M-
dc.date.accessioned2009-06-22T15:05:24Z-
dc.date.available2009-06-22T15:05:24Z-
dc.date.issued1985-
dc.identifier.citationHayes, D. S., Pasinetti, L. E and Philip, Davis A.G eds., Calibration of fundamental stellar quantities., Proceedings of the 111th Symposium of the International Astronomical Union held at Villa Olmo, Como, Italy, May 24 - 29, 1984., pp. 381 - 383en
dc.identifier.isbn90-277-2110-6-
dc.identifier.urihttp://hdl.handle.net/2248/4565-
dc.description.abstractThe existence of a tight linear correlation between the stellar absolute magnitude Mv and the Mg II k-line emission width log WMg II k (km s/sup-1) is confirmed using IUE high-resolution (0.2 Å) data for 100 late-type stars.en
dc.language.isoenen
dc.publisherD.Reidel Publishingen
dc.relation.ispartofseriesInternational Astronomical Union Symposium; No. 111-
dc.relation.urihttp://adsabs.harvard.edu//abs/1985IAUS..111..381Pen
dc.subjectStellar Quantities Calibrationen
dc.subjectAstrometryen
dc.subjectAstronomical Photometryen
dc.subjectAstronomical Techniquesen
dc.subjectMg II k-line Emissionen
dc.subjectWilson-Bappu effecten
dc.titleThe Wilson-Bappu effect for Mg II k-line emission widthsen
dc.typeArticleen
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