The Wilson-Bappu effect for Mg II k-line emission widths

dc.contributor.author	Parthasarathy, M
dc.date.accessioned	2009-06-22T15:05:24Z
dc.date.available	2009-06-22T15:05:24Z
dc.date.issued	1985
dc.identifier.citation	Hayes, 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 - 383	en
dc.identifier.isbn	90-277-2110-6
dc.identifier.uri	http://hdl.handle.net/2248/4565
dc.description.abstract	The 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.iso	en	en
dc.publisher	D.Reidel Publishing	en
dc.relation.ispartofseries	International Astronomical Union Symposium; No. 111
dc.relation.uri	http://adsabs.harvard.edu//abs/1985IAUS..111..381P	en
dc.subject	Stellar Quantities Calibration	en
dc.subject	Astrometry	en
dc.subject	Astronomical Photometry	en
dc.subject	Astronomical Techniques	en
dc.subject	Mg II k-line Emission	en
dc.subject	Wilson-Bappu effect	en
dc.title	The Wilson-Bappu effect for Mg II k-line emission widths	en
dc.type	Article	en