Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF

Publikation: AndetAndet bidragForskning

  • Iary Davidzon
OriginalsprogEngelsk
Publikationsdato2017
StatusUdgivet - 2017

ID: 243194808