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Ish: Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions
The Chemical Composition of the Sun
M. Asplund, N. Grevesse, A. J. Sauval +1
MaqolaOchiq kirish200920 iqtibosABIThe Dust Content and Opacity of Actively Star‐forming Galaxies
Daniela Calzetti, L. Armus, R. C. Bohlin +3
MaqolaOchiq kirish200018 iqtibosABIFirst results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
Annalisa Pillepich, Dylan Nelson, Lars Hernquist +8
MaqolaOchiq kirish20174 iqtibosABIgrackle: a chemistry and cooling library for astrophysics
Britton Smith, Greg L. Bryan, Simon C. O. Glover +11
Maqola20164 iqtibosABISimulating cosmic structure formation with the <scp>gadget</scp>-4 code
Volker Springel, Rüdiger Pakmor, Oliver Zier +1
Maqola20214 iqtibosABIA nearby galaxy perspective on dust evolution
F. Galliano, Angelos Nersesian, S. Bianchi +13
Maqola20214 iqtibosABIENVIRONMENTAL DEPENDENCE OF THE KENNICUTT-SCHMIDT RELATION IN GALAXIES
Nickolay Y. Gnedin, Andrey V. Kravtsov
MaqolaOchiq kirish20113 iqtibosABIGalaxy simulation with dust formation and destruction
Shohei Aoyama, Kuan-Chou Hou, Ikkoh Shimizu +4
Maqola20163 iqtibosABIOsaka feedback model: isolated disc galaxy simulations
Ikkoh Shimizu, Keita Todoroki, Hidenobu Yajima +1
Maqola20193 iqtibosABI