Talk:Galaxy morphological classification
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Van Den Bergh Luminosity Class
[edit]The article doesn't mention the Van Den Bergh luminosity class and I don't see it mentioned elsewhere on Wikipedia. Could that be covered? Praemonitus (talk) 00:43, 19 December 2021 (UTC)
Suitability of non-parametric galaxy morphology for this page
[edit]Hello,
I am wondering if a section on computational galaxy morphological parameters would be appropriate for this page. I understand that parameters like Concentration-Asymmetry-Smoothness and Gini-M20 are not quite the same as the hubble system, but I imagine readers hoping to learn about morphology to conduct research would be well served if this page referenced those concepts. Thank you! Jacobyuzov (talk) 01:56, 13 February 2026 (UTC)
Wiki Education assignment: PHY381 History of Modern Physics
[edit]
This article was the subject of a Wiki Education Foundation-supported course assignment, between 9 February 2026 and 27 April 2026. Further details are available on the course page. Student editor(s): Jacobyuzov (article contribs).
— Assignment last updated by Chrismazz1234 (talk) 05:03, 8 March 2026 (UTC)
CVRHS Classification System
[edit]For completeness, I'd like to suggest that this article should cover the Comprehensive de Vaucouleurs revised Hubble-Sandage (CVRHS) Classification System, as extended by Buta (2015) to "include other features such as inner, outer and nuclear lenses, nuclear rings and bars, bar ansae, barlenses, X patterns, thick discs, extraplanar discs and other features." Thank you. Praemonitus (talk) 20:33, 20 April 2026 (UTC)