Deciphering the radio-star formation correlation on kpc scales - IV. Radio halos of highly inclined spiral galaxies in the Virgo cluster

Open Access

Table 1.

Galaxy sample.

	D	i	S_4.85 GHz	$f_{4.85 GHz}^{therm}$ $f^{\mathrm{therm}}_{4.85\,\mathrm{GHz}}$	S_1.4 GHz	$f_{1.4 GHz}^{therm}$ $f^{\mathrm{therm}}_{1.4\,\mathrm{GHz}}$	SI	D_4.85 GHz	SFR	log(M_*)
	(Mpc)	(deg)	(mJy)		(mJy)			(kpc)	(M_⊙ yr⁻¹)	(M_⊙)
NGC4178	17	70	13.0	0.07	30.7	0.04	−0.69	23.5	0.8	9.6
NGC4192	17	78	35.0	0.21	120.9	0.06	−1.00	30.5	1.8	10.7
NGC4294	17	70	11.5	0.17	32.3	0.09	−0.83	12.8	0.5	9.2
NGC4419	17	74	23.6	0.32	59.8	0.14	−0.74	10.7	1.4	10.2
NGC4532	17	70	51.2	0.11	119.9	0.06	−0.68	15.2	1.3	9.2
NGC4808	17	68	19.4	0.22	62.6	0.08	−0.94	13.2	0.9	9.5

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