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Иш: Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions
On Dust Extinction of Gamma‐Ray Burst Host Galaxies
Aigen Li, S. L. Liang, Д. А. Канн +3
Мақола20082 иқтибосABIGas-to-dust mass ratios in local galaxies over a 2 dex metallicity range
A. Rémy-Ruyer, S. C. Madden, F. Galliano +17
Мақола20142 иқтибосABIWhat determines the grain size distribution in galaxies?
Ryosuke S. Asano, Tsutomu T. Takeuchi, Hiroyuki Hirashita +1
Мақола20132 иқтибосABIEFFICIENT THREE-DIMENSIONAL NLTE DUST RADIATIVE TRANSFER WITH SKIRT
M. Baes, J. Verstappen, Ilse De Looze +5
Мақола20112 иқтибосABIDust scaling relations in a cosmological simulation
Kuan-Chou Hou, Shohei Aoyama, Hiroyuki Hirashita +2
Мақола20192 иқтибосABIThe galactic dust-up: modelling dust evolution in FIRE
Caleb R Choban, Dušan Kereš, Philip F. Hopkins +3
Мақола20222 иқтибосABIInterstellar extinction in the Large Magellanic Cloud
K. Nandy, D. H. Morgan, A. J. Willis +2
Мақола19812 иқтибосABIFitting the integrated spectral energy distributions of galaxies
Jakob Walcher, Brent Groves, Tamás Budavári +1
Мақола20102 иқтибосABIUV to submillimetre luminosity functions of TNG50 galaxies
Ana Trc̆ka, M. Baes, Peter Camps +7
Мақола20222 иқтибосABI