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Table 4.
Large-scale magnetic fields in the halo.
| Source | Vertical | RMTL(b) | Magnetic field | Δ RMTL(c) | Hubble type(d) | SFR(e) |
|---|---|---|---|---|---|---|
| detection(a) | orientation | |||||
| [kpc] | [kpc] | |||||
| NGC 660 | 1.7 | SBa | 3.3 | |||
| NGC 891 | 2.5 | Sb | 1.9 | |||
| NGC 2820 | 2.9 | Yes | Horizontal | 2.0 | SBc | 1.4 |
| NGC 3044 | 3.3 | Yes | Vertical | 2.2 | SBc | 1.8 |
| NGC 3079 | 4.9 | SBcd | 5.1 | |||
| NGC 3448 | 2.7 | Possible | Possibly vertical | S0-a | 1.8 | |
| NGC 3556 | 2.5 | SBc | 3.6 | |||
| NGC 3735 | 4.6 | Possible | Horizontal | Sc | 6.2 | |
| NGC 4157 | 2.5 | Yes | Horizontal | 2.2 | SABb | 1.8 |
| NGC 4192 | 1.3 | Yes | Horizontal | 1.3 | SABb | 0.8 |
| NGC 4217 | 3.1 | Yes | Horizontal | 2.4 | Sb | 1.9 |
| NGC 4388 | 2.4 | Sb | 2.4 | |||
| NGC 4631 | 2.8 | Yes | Vertical | 1.9(f) | SBcd | 2.6 |
| NGC 4666 | 5.3 | SABc | 10.5 | |||
| NGC 5775 | 5.4 | Sbc | 7.6 |
Notes.
(d)
From HYPERLEDA, as used in Irwin et al. (2012).
(e)
This is SFRrevised in Vargas et al. (2019).
(f)
In the northern half (as detected in Mora-Partiarroyo et al. 2019b).
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