Radial properties of dust in galaxies: Comparison between observations and isolated galaxy simulations

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Table 2.

Total stellar mass, star formation rate, total gas mass, molecular gas mass, and 12 + log(O/H) gradient for the four galaxies in this study.

NGC reference	log(M_*[M_⊙])	log (SFR[M_⊙ yr⁻¹])	log(M_HI[M_⊙])	log(M_H₂[M_⊙])	12 + log(O/H)
NGC 628	10.34	0.24	9.70	9.08	^(a)8.835–0.485 × r/R₂₅
NGC 5457	10.3	0.53	10.15	9.5	^(b)8.716–0.832 × r/R₂₅
NGC 598	9.4	−0.40	9.15	8.52	^(c)8.50–0.382 × r/R₂₅
NGC 300	9.27	−0.82	9.32	7.67	^(d)8.57–0.41 × r/R₂₅

Notes.

^(a)

Berg et al. (2015),

^(b)

Croxall et al. (2016),

^(c)

Bresolin (2011),

^(d)

Toribio San Cipriano et al. (2016).

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