Notes. Given next to object and spectral type are distance (Col. 4), stellar effective temperature (Col. 5), stellar bolometric luminosity (Col. 6), stellar mass-loss rate (Col. 7), terminal stellar wind velocity (Col. 8), references of adopted stellar parameters (Col. 9), stellar-wind luminosity (Col. 10), bubble X-ray luminosity (Col. 11), hot-bubble radius (Col. 12), characteristic bubble temperature (Col. 13), and reference thereof (Col. 14). Distances based on the Gaia Data Release 3 (DR3), except for NGC 5315. Care was taken to ensure that all distance-dependent data are consistent with the distances given in Col. 4. The X-ray luminosities and X-ray temperatures refer to the energy range 0.3–2.0 keV (6.2–41.3 Å) and are from Ruiz et al. (2013) if not otherwise noted; T_X values derived from spectra of low quality are in italics. ^(a)Distance based on an assumed stellar luminosity of 4900 L_⊙; see text. ^(b)A new analysis performed by Todt (2019, priv. comm.) came up with a distance of 1 kpc for an extinction of E(B – V) = 0.85 and an assumed stellar luminosity of 6000 L_⊙. This distance is not compatible with the extinction-distance relation derived by Solf & Weinberger (1984), according to which the distance should be ≳2 kpc. Therefore, we kept the Gaia DR3 parallax and note that its error is 10% only (see text for more details).

References. (1) T_X value from Paper II; (2) T_X from Gruendl et al. (2006); (3) Marcolino et al. (2007); (4) Crowther et al. (2006); (5) de Freitas Pacheco et al. (1993); (6) Méndez et al. (1992); (7) Morisset & Georgiev (2009); (8) Kudritzki et al. (2006); (9) Pauldrach et al. (2004); (10) Toalá et al. (2019b); (11) Herald & Bianchi (2011); (12) Todt et al. (2015); (13) Georgiev et al. (2008); (14) Todt (2019, priv. comm.); (15) Keller et al. (2014); (16) Toalá et al. (2019a); (17) Toalá et al. (2020); (18) Guerrero et al. (2005).