Magnetic field in IRC+10216 and other C-rich evolved stars

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Table 1

Source list and observation parameters.

Object	Type	RA	Dec^a	d	V_LSR	L_bol	Ṁ	T_sys	rms
		[h m s]	[°′′′]	[pc]	[km s^-1]	[10³L_⊙]	[10^-6M_⊙/yr]	[K]	[mK]

IRC+10216	AGB	09 47 57.38	+13 16 43.7	120^d	–25.5	9.8^d	10–40^e	200–220	12–14
RW LMi	AGB	10 16 02.35	+30 34 19.0	400^d	–1.6	10^d	5.9^f	200–260	12
RY Dra	AGB	12 56 25.91	+65 59 39.8	431^d	–7.3	4.5^d	0.2^g	290–360	60
AFGL618	PPN	04 42 53.67	+36 06 53.2	900^a	–25.0	10-14^b	20–110^c	200	14
NGC 7027	PN	21 07 01.59	+42 14 10.2	980^h	25.0	7.2^h	N/A	230–250	14

Notes. The rms is for a velocity resolution of 0.2 km s^-1 in Stokes I.

^(a)

Sanchez Contreras & Sahai (2004).

^(b)

Knapp et al. (1993).

^(c)

Lee et al. (2013a,b).

^(d)

Ramstedt & Olofsson (2014).

^(e)

De Beck et al. (2012).

^(f)

De Beck et al. (2010).

^(g)

Cox et al. (2012).

^(h)

Zijlstra et al. (2008).

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