Deciphering the radio star formation correlation on kpc scales - I. Adaptive kernel smoothing experiments

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Table 1.

Galaxy sample.

Galaxy name	m_B	i^(a)	Dist ^(b)	Type	v_rot	Θ	B_ord ^(c)	B_turb
		(°)	(Mpc)		(km s⁻¹)	(″)	(μG)	(μG)
NGC 6946	9.76	18	6.0	SAB(rs)cd	200	18	9.9 ^(d)	12.6 ^(d)
M 51	9.26	33	8.4	SAbc	200	22	11.5 ^(e)	16.0 ^(e)
NGC 4321	10.02	27	17	SAB(s)bc	200	18	4.3	10.5
NGC 4303	9.97	25	17	SAB(rs)bc	200	18	6.5	15.4
NGC 4535	10.73	43	17	SAB(s)c	180	18	3.6	7.2
NGC 4254	10.44	20	17	SA(s)c	180	18	6.5 ^(f)	20.3 ^(f)
NGC 4501	10.50	57	17	SA(rs)b	260	18	7.1	15.3
NGC 4654	11.31	51	17	SAB(rs)cd	150	18	2.5	9.2

Notes.

^(a)

Inclination angle.

^(b)

This research has made use of the GOLD Mine Database (Gavazzi et al. 2003).

^(c)

The ordered magnetic field B_ord includes the large-scale ordered and the anisotropic small-scale magnetic fields.

^(d)

From Tabatabaei et al. (2013b).

^(e)

From Fletcher et al. (2011).

^(f)

Mean value based on Chyży (2008).

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