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Table 5
Modelling of the magnetization of the IGM.
| Type | Pri dSph | Pri dIrr | LBG | LBG | ||
| instantaneous star formation | ||||||
|
|
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| SF Mass | 2.0e5 | 1.0e7 | 4.0e8 | 4.0e9 | ||
| Redshift z | 8 | 7 | 5 | 3 | ||
| Wind energy Ew [erg] | 4.0e54 | 2.0e56 | 8.0e57 | 8.0e58 | ||
| SF size R0 [kpc] | 0.2 | 0.7 | 1.0 | 2.0 | ||
| Stall radius Rs [kpc] | 9 | 36 | 163 | 528 | ||
| B0 [G] | 1.0e-6 | 1.0e-5 | 2.3e-5 | 4.0e-5 | ||
| Bs [G] | 5.3e-10 | 1.9e-9 | 8.6e-10 | 5.7e-10 | ||
|
|
||||||
| Type | Local Group dIrrs | |||||
| continuous SF | ||||||
|
|
||||||
| SFR | 0.00001 | 0.0003 | 0.01 | 0.1 | ||
| Redshift z | 0 | 0 | 0 | 0 | ||
| Wind energy Ew [erg] | 3.0e50 | 1.5e52 | 3.0e53 | 3.0e54 | ||
| SF size R0 [kpc] | 0.05 | 0.2 | 0.4 | 0.7 | ||
| Stall radius Rs [kpc] | 0.2 | 0.9 | 2.3 | 5.0 | ||
| B0 [G] | 5.0e-7 | 1.0e-6 | 3.0e-6 | 8.0e-6 | ||
| Bs [G] | 2.3e-8 | 5.5e-8 | 8.8e-8 | 1.5e-7 | ||
Notes. From the assumed values of redshift z, TIGM, ϵ, R0, B0, SF mass or SFR, we first model Ew by the Starburst99 code and next obtain Rs and Bs (see the text for details).
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