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Table 3

Multiwavelength properties of galaxies from the literature.

Galaxy r25 rSB sini MHI log ΣHI M log ΣSFR 12 +log  (O/H) log ΣH2
kpc kpc 109M M pc-2 109M M yr-1 kpc-2 dex M pc-2
(2) (3) (4) (5) (6) (7) (8) (9) (10)

Haro 15 4.03 3.55 0.78 5.5 1.06 9.92 –1.28 8.33a <0.62h
Mrk 5 3.04 0.74 0.74 0.14 0.70 0.07 –1.72 8.10a <0.47i
Mrk 86 10.3 1.37 0.49 0.05 0.09 1.75 –1.70 8.53g 0.54k
Mrk 370 7.01 1.01 0.70 0.29 0.74 0.83 –1.66 8.51c 0.44i
Mrk 1089 6.04 3.82 0.79 7.46 1.51 3.38 –1.37 8.22d 0.61l
Mrk 1090 2.69 1.66 0.00 1.94 1.33 1.05 –0.92 8.15d <0.25m
UM 462 3.47 0.92 0.72 0.22 1.15 7.95 –0.80 7.99f 0.22j
I Zw 123 1.39 0.43 0.47 0.06 1.02 0.12 –1.12 7.86a <0.55i
II Zw 40 1.40 0.92 0.79 0.45 1.35 8.09 –0.69 8.07a 0.62n
II Zw 70 3.61 1.08 0.97 0.43 0.66 0.10 –1.70 7.69a <0.27m
II Zw 71 4.05 1.46 0.92 0.95 1.03 0.65 –1.77 8.24a 0.32p

Notes. Columns: (2) radius at the μB = 25 mag arcsec-2 isophote; (3) radius of the star-forming region from 2D surface photometry (Amorín et al. 2009); (4) inclination; (5) Hi gas mass; (6) logarithm of Hi gas surface density; (7) stellar mass; (8) logarithm of star-formation rate density; (9) gas-phase metallicity; (10) logarithm of H2 surface density assuming a Galactic CO-to-H2 conversion factor.

Reference. For metallicity: References for ΣH2:

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