CN Zeeman observations of the NGC 2264-C protocluster

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Table 1

CN(1–0) strong hyperfine lines.

Line	Frequency	Relative	Zeeman splitting	\|RI × Z\|^a
	(GHz)	intensity RI	factor Z (Hz/μG)

Z1	113.144	8	2.18	17.4
Z2	113.171	8	–0.31	2.5
Z3	113.191	10	0.62	6.2
Z4	113.488	10	2.18	21.8
Z5	113.491	27	0.56	15.1
Z6	113.500	8	0.62	5.0
Z7	113.509	8	1.62	13.0

Notes.

^(a)

| RI × Z | is the relative sensitivity to the magnetic field along the line of sight B_los.

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