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Иш: Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions
The Dust Content and Opacity of Actively Star‐forming Galaxies
Daniela Calzetti, L. Armus, R. C. Bohlin +3
Мақола200010 иқтибосABISimulating cosmic structure formation with the <scp>gadget</scp>-4 code
Volker Springel, Rüdiger Pakmor, Oliver Zier +1
Мақола20214 иқтибосABIGalaxy simulation with dust formation and destruction
Shohei Aoyama, Kuan-Chou Hou, Ikkoh Shimizu +4
Мақола20163 иқтибосABIgrackle: a chemistry and cooling library for astrophysics
Britton Smith, Greg L. Bryan, Simon C. O. Glover +11
Мақола20163 иқтибосABIOsaka feedback model: isolated disc galaxy simulations
Ikkoh Shimizu, Keita Todoroki, Hidenobu Yajima +1
Мақола20193 иқтибосABIA nearby galaxy perspective on dust evolution
F. Galliano, Angelos Nersesian, S. Bianchi +13
Мақола20213 иқтибосABI