Edithistory:Kormendy relation
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| oldid | date/time | username | edit summary |
|---|---|---|---|
| 1368609083 | 2026-08-10T02:12:32Z | Ldm1954 | [[WP:AFC|AFC]] draft |
| 1368609072 | 2026-08-10T02:12:31Z | Ldm1954 | Ldm1954 moved page [[Kormendy relation]] to [[Draft:Kormendy relation]]: [[WP:DRAFTIFY|Not ready]] for mainspace, incubate in draftspace. Reason/s: machine-generated |
| 1368548665 | 2026-08-09T18:47:53Z | Kowal2701 | add AI tag, see [[Wikipedia:AI noticeboard#User:Medelinezezie]] |
| 1364909765 | 2026-07-19T06:07:50Z | Vycl1994 | |
| 1364337961 | 2026-07-16T00:29:02Z | Praemonitus | +cat. |
| 1363888273 | 2026-07-13T02:50:46Z | Medelinezezie | |
| 1363887943 | 2026-07-13T02:48:03Z | Medelinezezie | [[WP:AES|←]]Created page with '{{Short description|Empirical relation between galaxy size and surface brightness}} {{Use American English|date=July 2026}} {{Use mdy dates|date=July 2026}} [[File:M105, NGC 3379 (noao-m105).jpg|thumb|right|300px|[[Messier 105]], an [[elliptical galaxy]]. Measurements of an elliptical galaxy's size and surface brightness can be placed on the Kormendy relation.]] The '''Kormendy relation''' is an empirical [[galaxy scaling relation|scaling relation]] betwe...' |
