Table 1
Model parameters and results.
Model | |||||||||||||||
name | Mlum | Reff | ν | τ | tgw | [⟨ Mg/Fe ⟩ ∗] | C, O yields | N | Stellar | Recipe | τ0 | QSO | MBH,seed | τBH | BEL |
(M⊙) | (kpc) | (Gyr-1) | (Gyr) | (Gyr) | primary | dust | dust | (M⊙) | (Gyr) | metall. | |||||
|
|||||||||||||||
M9 | 109 | 0.4 | 1.2 | 0.8 | 1.2 | +0.28 | François | no | off | – | – | – | – | – | – |
M9d | 109 | 0.4 | 1.2 | 0.8 | 1.2 | +0.28 | François | no | on | this work | 0.1 | off | – | – | – |
M10 | 1010 | 1 | 3 | 0.5 | 1.1 | +0.29 | François | no | off | – | – | – | – | – | – |
M10d | 1010 | 1 | 3 | 0.5 | 1.1 | +0.29 | François | no | on | this work | 0.08 | off | – | – | – |
M310 | 3 × 1010 | 2 | 5 | 0.5 | 1.0 | +0.30 | François | no | off | – | – | – | – | – | – |
M310N | 3 × 1010 | 2 | 5 | 0.5 | 1.0 | +0.30 | François | yes | off | – | – | – | – | – | |
M310d | 3 × 1010 | 2 | 5 | 0.5 | 1.0 | +0.30 | François | no | on | this work | 0.05 | off | – | – | – |
M310Nd | 3 × 1010 | 2 | 5 | 0.5 | 1.0 | +0.30 | François | yes | on | this work | 0.05 | off | – | – | – |
M310Cd | 3 × 1010 | 2 | 5 | 0.5 | 1.0 | +0.30 | François | no | on | Calura | 0.05 | off | – | – | – |
M310MD | 3 × 1010 | 2 | 5 | 0.5 | 1.0 | +0.30 | Maeder | no | off | – | – | – | – | – | – |
M310MDd | 3 × 1010 | 2 | 5 | 0.5 | 1.0 | +0.30 | Maeder | no | on | this work | 0.01 | off | – | – | – |
M11 | 1011 | 3 | 10 | 0.4 | 0.9 | +0.33 | François | no | off | – | – | – | – | – | – |
M11d | 1011 | 3 | 10 | 0.4 | 0.9 | +0.33 | François | no | on | this work | 0.03 | on | – | – | – |
M12 | 1012 | 10 | 20 | 0.2 | 0.7 | +0.39 | François | no | off | – | – | – | – | – | – |
M12d | 1012 | 10 | 20 | 0.2 | 0.7 | +0.39 | François | no | on | this work | 0.01 | on | 2 × 103 | 0.049 | mod |
M12MDd | 1012 | 10 | 20 | 0.2 | 0.7 | +0.39 | Maeder | no | on | this work | 0.01 | on | 2 × 103 | 0.049 | mod |
M12dcaseA | 1012 | 10 | 20 | 0.2 | 0.7 | +0.39 | François | no | on | this work | 0.01 | on | 2 × 103 | 0.049 | 5x |
M12dcaseB | 1012 | 10 | 20 | 0.2 | 0.7 | +0.39 | François | no | on | this work | 0.01 | on | 4 × 103 | 0.049 | mod |
M12dcaseC | 1012 | 10 | 20 | 0.2 | 0.7 | +0.39 | François | no | on | this work | 0.01 | on | 8 × 103 | 0.049 | mod |
M12dcaseD | 1012 | 10 | 20 | 0.2 | 0.7 | +0.39 | François | no | off | – | 0.01 | on | 1 × 108 | 0.49 | mod |
Notes. The values for tgw and [⟨ Mg/Fe ⟩] refer to the central regions of the galaxy. These values are determined only by Mlum (and hence by ν and τ). At each given mass models differ by C, O and N yields – fiducial, Maeder (1992) and primary production, respectively – dust (on/off, prescriptions for stellar dust, τ0 and QSO dust production). The BEL metallicity is the metallicity of the gas out of which the QSO dust forms: mod refer to a model self-consistently calculated metallicity, 5x is for the case in which the adopted metallicity is 5 times higher than the average mod one.
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.