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Table 9

Parameters for the star formation law.

Galaxy Metal. M(H i) M(H2) SFR Area
[O/H] [log M] [log M] [M yr-1] [kpc2]
(1) (2) (3) (4) (5) (6)

Haro 11 8.20 8.70 9.40 27.6 1266
Mrk 1089 8.10 10.2 9.65 5.11 1350
Mrk 930 8.03 9.50 8.83 2.80 1617
NGC 4861 7.89 8.62 <8.04 0.048 60
NGC 625 8.22 8.04 7.65 0.042 32
UM 311 8.38 9.48 8.61 0.77 834

Additional DGS compact galaxies

Haro 2 8.23 8.58 9.07 0.95 87
Haro 3 8.28 9.05 8.55 0.80 99
He 2-10 8.43 8.49 8.52 0.68 65
I Zw 18 7.14 8.00 <8.85 0.005 4.8
Mrk 209 7.74 7.43 8.47 0.005 1.4
NGC 5253 8.25 8.02 7.37 0.26 17
SBS 0335-052 7.25 8.64 <10.4 0.26 23
UM 448 8.32 9.78 10.3 13.4 2332
UM 461 7.73 7.86 <9.49 0.014 3.7
VII Zw 403 7.66 7.52 <8.79 0.003 2.4

Notes. (1) Galaxy name; (2) metallicities from Madden et al. (2013); (3) aperture-corrected H i masses assuming an exponential distribution, from Rémy-Ruyer et al. (2014); (4) H2 masses using XCO,Z. CO data are from: Israel et al. (1995) for Haro 2; Tacconi & Young (1987) for Haro 3 and Mrk 209; Kobulnicky et al. (1995) for He 2-10; Leroy et al. (2005) for I Zw 18 and VII Zw 403; Taylor et al. (1998) for NGC 5253; Dale et al. (2001) for SBS 0335-052; and Sage et al. (1992) for UM 448 and UM 461. (5) Star formation rate using LTIR from Rémy-Ruyer et al. (in prep.) and the formula from Murphy et al. (2011); (6) area defined from the Herschel photometry apertures (Rémy-Ruyer et al. 2013) and using distances from Madden et al. (2013).

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