Measuring magnetic fields from water masers in the synchrotron protostellar jet in W3(H2O)

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Table 1

Measurements of the magnetic field strength from H₂O masers with Zeeman splitting in TW-A.

Maser	RA (J2000)	Dec (J2000)	B strength	R ^a
ID	(h:m:s)	(^o:’:")	(mG)	(arcsec)

037	02:27:04.7444	61:52:24.694		0.347
051	02:27:04.7409	61:52:24.705		0.314
104	02:27:04.6994	61:52:24.655		0.110
105	02:27:04.6993	61:52:24.656		0.111

Notes.

^(a)

Sky-projected separation between the masers with Zeeman splitting measurements and the putative location of the TW-A protostar, estimated from the peak of the 8.4 GHz continuum, α₂₀₀₀ = 02^h27^m04^s.7103 and δ₂₀₀₀ = + 061°52′24′′.650.

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