Open Access

Table 1.

PHANGS–ALMA galaxies studied in this work, their properties, and the number of superbubbles found within them from Leroy et al. (2021b).

Galaxy Distance (a) No. of SFR Mstar MH I MH2
(Mpc) bubbles (M yr−1) (109 M) (109 M) (109 M)
NGC 0628 9.84 34 1.8 21.9 5.0 4.7
NGC 1087 15.85 15 1.3 8.6 1.3 1.7
NGC 1300 18.99 11 1.2 41.4 2.4 3.2
NGC 1365 19.57 6 16.9 97.8 8.7 24.6
NGC 1385 17.22 12 2.1 9.5 1.6 1.8
NGC 1433 18.63 12 1.1 73.4 2.5 2.7
NGC 1512 18.83 15 1.3 51.6 7.6 1.9
NGC 1566 17.69 31 4.5 60.9 6.4 6.2
NGC 1672 19.40 13 7.6 53.6 16.0 9.1
NGC 2835 12.22 6 1.2 10.0 3.0 1.0
NGC 3351 9.96 13 1.3 23.0 0.8 1.9
NGC 3627 11.32 39 3.8 68.1 1.2 7.0
NGC 4254 13.10 37 3.1 26.6 3.0 8.2
NGC 4303 16.99 24 5.3 33.4 4.6 11.4
NGC 4321 15.21 25 3.6 55.6 2.7 9.7
NGC 4535 15.77 16 2.2 34.0 3.7 7.1
NGC 5068 5.20 6 0.3 2.5 0.7 0.4
NGC 7496 18.72 10 2.3 9.9 1.2 2.1

Notes. SFR is the star formation rate, Mstar is the stellar mass, MH I is the mass of neutral hydrogen, and MH2 is the mass of molecular hydrogen for the entire galaxy.

(a)

Distances from Anand et al. (2021), also see acknowledgements.

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