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- W1600816211 abstract "We address the origin of the robustly observed bi‐modality in galaxy properties at a characteristic stellar mass of ∼ 3 × 10 10M⊙. As seen in large surveys at low redshift and indicated at z ∼ 1, less massive galaxies tend to be star‐forming blue (some very blue) discs in the “field”, correlated along a “fundamental line” of L/M, surface brightness, internal velocity and metallicity rising with mass. More massive galaxies are mostly spheroids of red (some very red) old stars in groups or clusters, with surface brightness and metallicity ∼constant and halo M/L rising with mass. The spheroids tend to host AGNs.We propose that the bi‐modality is the combined effect of the thermal history of the infalling gas and several feedback processes, aided by the gravitational growth of fluctuations into groups of galaxies. In haloes below a critical mass ∼ 10 12M⊙, single discs are built by cold streams, not heated by a shock in the extended dark halo, yielding efficient early star formation. It is regulated by supern..." @default.
- W1600816211 created "2016-06-24" @default.
- W1600816211 creator A5017176794 @default.
- W1600816211 date "2004-01-01" @default.
- W1600816211 modified "2023-10-17" @default.
- W1600816211 title "Characteristic Scale and Bimodality in Galaxies: Cold Streams, Shock Heating, Feedback and Clustering" @default.
- W1600816211 doi "https://doi.org/10.1063/1.1848326" @default.
- W1600816211 hasPublicationYear "2004" @default.
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