Table 1
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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.