Relative distribution of dark matter, gas, and stars around cosmic filaments in the illustristng simulation

HIGHLIGHTS

• who: Galu00e1rraga-Espinosa Daniela and colleagues from the Universitu00e9 Paris-Saclay, CNRS, Institut d`astrophysique spatiale, Orsay, France have published the Article: Relative distribution of dark matter, gas, and stars around cosmic filaments in the IllustrisTNG simulation, in the Journal: (JOURNAL)
• what: The authors show that the large-scale environment (i.e. denser versus less dense hotter versus colder regions) has non-negligible effect on the absolute values of the DM gas and stellar densities around filaments. The authors provide scaling relations between the gas density temperature and pressure for the different populations of cosmic . . .
  

   

  

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