Table 5
Projected magnetic field strength on the star surface.
| Source | R∗ | BH2Omin | B H2Omax |
|
|
B starmin | B starmax | B starmin | B starmax | B starmin | B starmax | |
| (AU) | (mG) | (mG) | (AU) | (AU) | (G) | (G) | (G) | (G) | (G) | (G) | ||
| (α=1) | (α = 1) | (α = 2) | (α = 2) | (α = 3) | (α = 3) | |||||||
|
|
||||||||||||
| IK Tau | 2.8 | 65 | 271 | 22.5 | 27.8 | 0.5 | 2.7 | 4.2 | 26.8 | 33.8 | ~265 | |
| RT Vir | 0.8 | 131 | 194 | 6.0 | 14.6 | 1.0 | 3.5 | 7.3 | 64.9 | 54.9 | ~1185 | |
| IRC+60370 | 1.8 | 44 | 413 | 12.5 | 29.5 | 0.3 | 6.9 | 2.2 | ~115 | 15.8 | ~1945 | |
Notes.From Cols. 1 to 12: the source name (Source), the stellar radius (R∗), the lower (BH2Omin) and upper (BH2Omax) magnetic field strengths along the line of sight observed in the H2O region, the input values of R on Eq. (4) ( and ), and the lower (Bstarmin) and upper (Bstarmax) limits of the projected magnetic field strength on the stellar surface assuming α = 1, α = 2, and α = 3.
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