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Table 3.
Velocity range and upper limits on the dipolar magnetic field derived using the marginal (MD) and definite (DD) detection criteria for each star.
| Source ID | Velocity range | max(Bpol) (G) | |
|---|---|---|---|
| (km s−1) | (MD) | (DD) | |
| V806 Tau | −30/40 | 1900 | 3700 |
| MHO 3 | −50/60 | 4900 | > 5000 |
| MHO 2 | −16/40 | 3000 | 4300 |
| IRAS 04292+2422 W | 15/40 | 480 | 650 |
| IRAS 04113+2758 N | −6/30 | 1900 | 2300 |
| IRAS 04369+2539 | −30/60 | > 5000 | > 5000 |
| HL Tau | −40/65 | 4900 | > 5000 |
| IRAS 16191–1936 | −30/40 | > 5000 | > 5000 |
| L1689 SNO2 | −45/25 | 2500 | 4100 |
| IRAS 03247+3001 | −60/60 | > 5000 | > 5000 |
| V512 Per | −10/30 | 3300 | 4100 |
| VV CrA SW | −20/20 | > 5000 | > 5000 |
| VV CrA NE | −25/20 | 4700 | > 5000 |
| SVS 20 S | −70/60 | > 5000 | > 5000 |
Notes. The detected magnetic protostars are indicated in bold font.
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