Physical properties of the three simulations representative of various galaxy types in this work.
|Model||M ∗||f gas||Redshift||⟨ sSFR ⟩|
|spiral||6.5 × 1010 M⊙||9%||z = 0||0.04 Gyr-1|
|SB merger||6.5 × 1010 M⊙ (×2)||9%||z = 0||0.63 Gyr-1|
|high-z disk||3.5 × 1010 M⊙||60%||z = 2||0.97 Gyr-1|
Notes. The specific star formation rate (sSFR) indicated here is averaged over the snapshots analyzed for each galaxy type: random for the spiral and high-z disk model, picked only in starbursting phases for the SB merger model. The stellar mass and gas fraction are the initial parameters of the models. A representative redshift is indicated for each model and is also used as an input parameter for the CMB temperature in the LVG grids.
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