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Иш: Radial properties of dust in galaxies: Comparison between observations and isolated galaxy simulations
Simulating 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 иқтибосABITHINGS: THE H I NEARBY GALAXY SURVEY
Fabian Walter, E. Brinks, W. J. G. de Blok +4
Мақола20082 иқтибосABIDust grains from the heart of supernovae
M. Bocchio, S. Marassi, R. Schneider +3
Мақола20162 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 иқтибосABIThe CO-to-H<sub>2</sub> Conversion Factor
Alberto D. Bolatto, M. G. Wolfire, Adam K. Leroy
Мақола20132 иқтибосABI