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Mark Naoumides's Unpublished Papers on Cyril's Lexicon: An Initial Overview with Some Remarks on the g-Recension
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Astrophysics > Astrophysics of Galaxies
The total mass distribution in galaxies strongly influences star formation (SF), both directly via gas availability and feedback, and indirectly via the dark matter (DM) potential well. Star formation efficiency peaks at a characteristic stellar mass of $5 \times 10^{10} M_{\odot}$, often termed the "golden mass", where feedback mechanisms minimally affect SF.
Astrophysics > Astrophysics of Galaxies
[Submitted on 4 Nov 2026] Title:Quiescent galaxies at cosmic noon: from individual element abundances to star formation histories Authors:M. Longhetti , F.R. Ditrani , D. Bevacqua , G. De Lucia , A. Gallazzi , A. Gargiulo , F. La Barbera , C. Maraston , D. Thomas , P. Franzetti , C. Mancini , L. Scholz-Díaz , S. Zibetti View a PDF of the paper titled Quiescent galaxies at cosmic noon: from individual element abundances to star formation histories, by M.
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