The resolved scaling relations in DustPedia: Zooming in on the local Universe

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Volume 668 (December 2022)

A&A, 668 (2022) A130

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Table 2.

Global masses and SFR of galaxies.

Galaxy	log(M_star) ⁽¹⁾	log(M_H2) ⁽²⁾	log(M_HI) ⁽³⁾	log(M_dust) ⁽¹⁾	SFR ⁽¹⁾
	[M_⊙]	[M_⊙]	[M_⊙]	[M_⊙]	[M_⊙ yr⁻¹]
NGC 300	9.34 ± 0.18	–	9.28 ± 0.03	6.70 ± 0.18	0.20 ± 0.03
IC 342	10.31 ± 0.09	9.70 ± 0.14	10.02	7.35 ± 0.04	4.03 ± 0.26
NGC 2403	9.47 ± 0.07	8.25 ± 0.14	9.41 ± 0.02	6.64 ± 0.04	0.73 ± 0.05
NGC 3031 (M 81)	10.65 ± 0.06	8.12 ± 0.13	9.55 ± 0.02	7.02 ± 0.07	0.35 ± 0.13
NGC 7793	9.29 ± 0.13	8.10 ± 0.15	8.91 ± 0.02	6.56 ± 0.04	0.46 ± 0.03
NGC 4736 (M 94)	10.39 ± 0.07	8.61 ± 0.14	8.55 ± 0.02	6.39 ± 0.03	0.55 ± 0.19
NGC 6946	10.43 ± 0.14	9.94 ± 0.14	9.73 ± 0.02	7.48 ± 0.08	7.07 ± 0.56
NGC 5236 (M 83)	10.50 ± 0.11	9.85 ± 0.14	9.31 ± 0.02	7.30 ± 0.12	6.66 ± 1.09
NGC 3621	10.31 ± 0.12	8.34 ± 0.13 ⁽⁵⁾	9.86 ± 0.02	7.03 ± 0.05	1.42 ± 0.23
NGC 5457 (M 101)	10.15 ± 0.06	9.55 ± 0.13	10.12 ± 0.02	7.67 ± 0.05	4.75 ± 0.24
NGC 5194 (M 51)	–⁽⁴⁾	9.55 ± 0.13 ⁽⁵⁾	9.55	–⁽¹⁾	– ⁽⁴⁾
NGC 5055 (M 63)	10.77 ± 0.08	9.62 ± 0.14	9.86 ± 0.02	7.65 ± 0.08	2.46 ± 0.74
NGC 925	9.73 ± 0.12	< 8.14	9.72 ± 0.00	6.97 ± 0.04	1.15 ± 0.07
NGC 628 (M 74)	10.15 ± 0.07	8.91 ± 0.14	10.01 ± 0.00	7.58 ± 0.14	2.41 ± 0.45
NGC 3521	10.93 ± 0.08	9.53 ± 0.15	9.93 ± 0.00	7.73 ± 0.03	3.15 ± 1.26
NGC 4725	10.87 ± 0.07	8.74 ± 0.51	9.60 ± 0.00	7.39 ± 0.05	0.93 ± 0.11
NGC 1365	10.92 ± 0.14	10.00 ± 0.13	9.98 ± 0.03	8.00 ± 0.15	12.97 ± 4.97
NGC 1097	10.99 ± 0.11	9.79 ± 0.13	9.91 ± 0.07	7.57 ± 0.10	6.56 ± 1.05

Notes.

⁽¹⁾

M_star, M_dust, and SFR values from Bianchi et al. (2018) and Nersesian et al. (2019) obtained through the modeling of the galaxy SED with CIGALE code (Boquien et al. 2019).

⁽²⁾

M_H2 values from C20 derived within r₂₅ under the assumption of a constant X_CO (Bolatto et al. 2013).

⁽³⁾

M_HI values from De Vis et al. (2019).

⁽⁴⁾

NGC 5194 lacks M_star, M_dust, and SFR values because it has not been fitted by CIGALE.

⁽⁵⁾

M_H2 values derived from maps used in this work under the same assumptions of C20.

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