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Table 1.

Properties of the galaxy sample.

Galaxy RA Dec i PA Morph. Dist. Scale Reff VLSR MHI MH2 Mstar SFR
° ° ° ° Mpc pc/″ kpc km/s log(M) log(M) log(M) M yr−1
(a) (b) (b) (c) (c) (d) (e) (f) (g) (h) (i) (j) (k) (l)
NGC 3627 170.063 12.991 57.3 173.1 Sb 11.3 55 3.6 715.4 9.1 9.8 10.8 3.8
NGC 4321 185.729 15.822 38.5 156.2 SABb 15.2 70 5.5 1572.3 9.4 9.9 10.7 3.6
NGC 6946 308.719 60.154 33.0 243.0 SABc 7.3 34 4.5 61.3 10.0 9.6 10.5 5.9

Notes. (a) Galaxy name. (b) Central right ascension (RA) and declination (Dec) from Salo et al. (2015). (c) Position angle (PA) from de Blok et al. (2008), Lang et al. (2020). (d) Morphological (Morph.) classification taken from HyperLEDA (Makarov et al. 2014). (e) Source distances (Dist.) are taken from the compilation of Anand et al. (2021a,b). (f) Distance scale. (g) Effective radius (Reff) that contains half of the stellar mass of the galaxy (Leroy et al. 2021). (h) Centroid velocity (VLSR). Local standard of rest velocities taken from HyperLEDA (Makarov et al. 2014) and Lang et al. (2020). (i) Total atomic gas mass (MHI) taken from HYPERLEDA (Makarov et al. 2014). (j) Total molecular gas mass (MH2) from Leroy et al. (2013). (k) Stellar mass (Mstar) from Leroy et al. (2021). (l) Global star formation rate (SFR) derived by Leroy et al. (2021), using GALEX UV and WISE IR photometry, following a similar methodology to Leroy et al. (2019).

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