CHANG-ES - XXXVI. The thin and thick radio discs | Astronomy & Astrophysics (A&A)

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Volume 699 (July 2025)

A&A, 699 (2025) A243

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Table A.1.

Properties of galaxies in the sample.

Galaxy	d	log₁₀r_★	log₁₀ Σ_SFR	log₁₀ Σ_tot	log₁₀ (Σ_SFR/Σ_tot)	SFR	i	pa
	(Mpc)	(kpc)	(M_⊙ yr⁻¹ kpc⁻²)	(M_⊙ kpc⁻²)	(yr⁻¹)	(M_⊙ yr⁻¹)	(°)	(°)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
N0891	9.1	1.10	−2.42	8.39	−10.81	1.88	84	22
N2683	6.27	0.67	−2.44	8.72	−11.16	0.25	79	44
N2820	26.5	0.84	−2.04	8.34	−10.38	1.35	88	65
N3003	25.4	1.14	−2.59	7.77	−10.35	1.56	85	79
N3044	20.3	0.96	−2.17	8.24	−10.41	1.75	85	−67
N3079	20.6	1.11	−2.02	8.30	−10.31	5.08	88	−14
N3432	9.42	0.70	−2.18	8.17	−10.35	0.51	85	41
N3448	24.5	0.79	−1.84	8.42	−10.25	1.78	78	65
N3556	14.09	1.10	−2.14	7.98	−10.12	3.57	81	79
N3628	8.5	1.09	−2.52	8.32	−10.85	1.41	87	−76
N3735	42.0	1.24	−2.18	8.26	−10.43	6.23	85	−50
N4013	16.0	0.90	−2.46	8.35	−10.80	0.71	88	65
N4096	10.32	0.77	−2.19	8.34	−10.53	0.71	82	20
N4157	15.6	0.92	−2.09	8.38	−10.47	1.76	83	65
N4217	20.6	1.07	−2.36	8.28	−10.64	1.89	86	50
N4302	19.41	1.03	−2.60	8.25	−10.85	0.92	90	−2
N4388	16.6	0.74	−1.60	8.57	−10.17	2.42	79	−89
N4565	11.9	1.26	−3.03	7.89	−10.92	0.96	86	−45
N4631	7.4	1.07	−2.21	7.98	−10.19	2.62	85	86
N4666	27.5	1.21	−1.89	8.20	−10.09	10.5	76	41
N5775	28.9	1.20	−2.03	8.17	−10.20	7.56	86	−35
N5907	16.8	1.25	−2.66	8.13	−10.79	2.21	90	−24

Notes. Column (2) d is the distance (Wiegert et al. 2015); (3) r_★ is the star formation radius as from near infrared (Wiegert et al. 2015); (4) is the SFR surface density within r_★; (5) total mass surface density from Irwin et al. (2012a) scaled to our distances (6) ratio of SFR-to-mass surface density; (7) star formation rate from Hα and mid-infrared (Vargas et al. 2019); (8) inclination and position angles from Krause et al. (2018, N2820, 3003, 3044, 3079, 3432, 3735, 3877, 4013, 4157, 4217, 4302, 5775), otherwise Irwin et al. (2012a); (9) position angle from Krause et al. (2018, see inclination angle), otherwise Hyperleda

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