← Назад к работе
Работы, на которые ссылается эта работа
Работ: 134
Работа: Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions
The relationship between infrared, optical, and ultraviolet extinction
Jason A. Cardelli, Geoffrey C. Clayton, John S. Mathis
Статья1989Цитирований: 36ABIThe Chemical Composition of the Sun
M. Asplund, N. Grevesse, A. J. Sauval +1
Статья2009Цитирований: 15ABIThe Dust Content and Opacity of Actively Star‐forming Galaxies
Daniela Calzetti, L. Armus, R. C. Bohlin +3
Статья2000Цитирований: 10ABISimulating cosmic structure formation with the <scp>gadget</scp>-4 code
Volker Springel, Rüdiger Pakmor, Oliver Zier +1
Статья2021Цитирований: 4ABIThe EAGLE project: simulating the evolution and assembly of galaxies and their environments
Joop Schaye, Robert A. Crain, R. G. Bower +19
Статья2014Цитирований: 4ABISKIRT: An advanced dust radiative transfer code with a user-friendly architecture
Статья2014Цитирований: 3ABIGalaxy simulation with dust formation and destruction
Shohei Aoyama, Kuan-Chou Hou, Ikkoh Shimizu +4
Статья2016Цитирований: 3ABIgrackle: a chemistry and cooling library for astrophysics
Britton Smith, Greg L. Bryan, Simon C. O. Glover +11
Статья2016Цитирований: 3ABIOsaka feedback model: isolated disc galaxy simulations
Ikkoh Shimizu, Keita Todoroki, Hidenobu Yajima +1
Статья2019Цитирований: 3ABIA nearby galaxy perspective on dust evolution
F. Galliano, Angelos Nersesian, S. Bianchi +13
Статья2021Цитирований: 3ABIInfrared Emission from Interstellar Dust. I. Stochastic Heating of Small Grains
Статья2001Цитирований: 3ABI