Clumps in high-redshift spiral galaxies are smaller than commonly reported, spatially concentrated toward spiral arms, smaller but brighter inside arms than between them, with similar colors, suggesting arms stimulate clump formation but do not alter their star formation properties.
and Zhou, YanYan , year =
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Plasmoid reconnection simulations match observed skewness transitions and entropy decreases in FSRQ GeV light curves after flares, with broken power-law PSDs consistent with blazar variability.
citing papers explorer
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Clumps in spiral galaxies at $z \lesssim 3$: Disentangling two spatial modes of star formation
Clumps in high-redshift spiral galaxies are smaller than commonly reported, spatially concentrated toward spiral arms, smaller but brighter inside arms than between them, with similar colors, suggesting arms stimulate clump formation but do not alter their star formation properties.
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Reconnection-driven State Transitions in Flat Spectrum Radio Quasars
Plasmoid reconnection simulations match observed skewness transitions and entropy decreases in FSRQ GeV light curves after flares, with broken power-law PSDs consistent with blazar variability.