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Table 2.

Properties of the sample galaxies.

Morphological Total apparent corrected Total Stellar Mass
Galaxy Type Distance (Mpc) Nuclear Activity PA (°) Bar PA (°) Inclination (°) B-magnitude (mag) log(M*/M)
NGC 1300 SB(rs)bc 14.5 LINER (AGN) 278a 1041 31.8a 10.61 10.307
NGC 1792 SA(rs)bc 11.3 HII Region 316 63.1 10.18 10.578
NGC 2903 SAB(rs)bc 8.57 HII Region 202 242 67.1 8.83 10.319
NGC 3059 SB(rs)bc 14.8 HII Region 330 393 21.3 10.63 10.408
NGC 4303 SAB(rs)bc 12.2 Seyfert 2/LINER 310 24 18.1 10.02 10.487
NGC 4321 SAB(s)bc 15.8 LINER (AGN) 156a 1084 24 9.83 10.7110
NGC 4536 SAB(rs)bc 14.7 LINER (AGN) 306a 1365 66a 10.27 10.1910
NGC 4689 SA(rs)bc 15.7 HII Region 163 42.5 11.23 10.588
NGC 5248 SAB(rs)bc 11.8 Seyfert/LINER 120 1274 56.4 10.39 10.3011
NGC 5921 SB(r)bc 17.3 HII Region 137 186 49.5 11.2 10.4112

Notes. The distances are medians of the values listed on NED and morphological types are from de Vaucouleurs et al. (1991). PA, Inclination, and the Total apparent corrected B band magnitude were obtained from Hyperleda (Makarov et al. 2014). The values for the PA and inclination of NGC 1300, NGC 4321 and NGC 4536 (indicated by “a”) are from Lang et al. (2020). The nuclear activity classifications are discussed in Appendix A.

References for the bar PA: (1) Lindblad et al. (1997), (2) Sheth et al. (2002), (3) Bottema (1990). (4) Das et al. (2003), (5) Shaw et al. (1995), (6) Martin & Friedli (1997). References for the total stellar mass: (7) Davis et al. (2019), (8) Weinzirl et al. (2009), (9) Murugeshan et al. (2020), (10) Zabel et al. (2022), (11) Chiang et al. (2024), (12) Díaz-García et al. (2021).

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