The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies

Author(s):: Chaikin, E.; Schaye, J. (0000-0002-0668-5560); Schaller, M. (0000-0002-2395-4902); Bahé, Y.M.; Nobels, F.S.J.; Ploeckinger, S.

Methods - numericalGalaxies - evolutionGalaxies - formationGalaxies - generalAstrophysics - astrophysics of galaxies

Date issued: 2022
Language: English
Is part of: Monthly Notices of the Royal Astronomical Society (2022), Vol. 514, no. 1, p. 249-264
hdl: 1887/3514431
doi: 10.1093/mnras/stac1132
URL: https://ui.adsabs.harvard.edu/abs/2022MNRAS.514..249C