The magnetic fields of large Virgo cluster spirals. II

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Table 1

Basic astronomical properties and parameters of radio observations of studied galaxies.

NGC	Morph.	Optical position^a		Incl.^a	Pos.	Dist. to	Number	rms in final map
	type^a	α ₂₀₀₀	δ ₂₀₀₀	[°]	ang.^a[°]	Vir A [°]	of cov.	[mJy/b.a.]
								TP	PI


4192	SABb	12^h13^m483	+14°53′ 57 7	78	152.5	4.84	20^c	0.3^c	0.09^c
							12^b	0.7^b	0.1^b
4302	Sc	12^h21^m425	+14°35′ 52 1	90	177.5	3.12	18^c	0.3^c	0.07^c
							11^b	0.8^b	0.08^b
4303	Sbc	12^h21^m550	+04°28′ 28 8	26.3	162	8.2	20^c	0.3^c	0.08^c
							14^b	1.1^b	0.1^b
4321	SABb	12^h22^m550	+15°49′ 21 3	30	130	3.9	21^c	0.3^c	0.07^c
							15^b	0.8^b	0.1^b
4388	Sb	12^h25^m468	+12°39′ 43 6	82	91.3	1.26	12^b	0.9^b	0.1^b
4535	SBc	12^h34^m204	+08°11′ 52 3	41.3	180	4.3	20^c	0.3^c	0.07^c

Notes.

^(a)

Taken from HYPERLEDA database – http://leda.univ-lyon1.fr – see Paturel et al. (1983);

^(b)

at 4.85 GHz;

^(c)

at 8.35 GHz.

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