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• W4280565571 abstract "We analyse measurements of the evolving stellar mass (ℳ 0 ) at which the bending of the star-forming main sequence (MS) occurs over 0 < z < 4. We find ℳ 0 ≈ 10 10 M ⊙ over 0 < z < 1 before ℳ 0 rises up to ∼10 11 M ⊙ at z = 2 and then stays flat or slowly increases towards higher redshifts. When converting ℳ 0 values into hosting dark matter halo masses, we show that this behaviour is remarkably consistent with the evolving cold- to hot-accretion transition mass, as predicted by theory and defined by the redshift-independent M shock at z < 1.4 and by the rising M stream at z ≳ 1.4 (for which we propose a revision in agreement with the latest simulations). We therefore argue that the MS bending is primarily due to a drop in cold accretion, causing a reduction in available cold gas in galaxies, which supports predictions of gas feeding theory. In particular, the rapidly rising ℳ 0 with redshift at z > 1 is evidence in favour of the cold-streams scenario. In this picture, a progressive fuelling reduction rather than its sudden suppression in halos more massive than M shock / M stream produces a nearly constant star-formation rate in galaxies with stellar masses larger than ℳ 0 , and not their quenching, which therefore requires other physical processes. Compared to the knee M * in the stellar mass function of galaxies, ℳ 0 is significantly lower at z < 1.5, and higher at z > 2, suggesting that the imprint of gas deprivation on the distribution of galaxy masses happened at early times ( z > 1.5–2). The typical mass at which galaxies inside the MS become bulge-dominated evolves differently from ℳ 0 , which is consistent with the idea that bulge formation is a distinct process from the phasing out of cold accretion." @default.
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• W4280565571 date "2022-05-01" @default.
• W4280565571 modified "2023-10-16" @default.
• W4280565571 title "The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0 < <i>z</i> < 4" @default.
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• W4280565571 doi "https://doi.org/10.1051/0004-6361/202243574" @default.
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