Photometric decomposition of edge-on galaxies indicates that projection effects cause a substantially higher fraction of Type II disk breaks than reported in previous work.
Photoelectric Photometry of Messier 33 IN the u, b, v, System
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A multiphase ISM grain-size model with low supernova dust yield reproduces observed dust-to-stellar mass ratios and UV luminosity functions at z=7-12 by letting small grains seed rapid metal accretion.
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Grain-size evolution and rapid dust growth in high-redshift galaxies
A multiphase ISM grain-size model with low supernova dust yield reproduces observed dust-to-stellar mass ratios and UV luminosity functions at z=7-12 by letting small grains seed rapid metal accretion.