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Table 1.

Properties of our sample of MaNGA galaxies with the off-centered spots of the enhanced gas velocity dispersion.

MaNGA Other RA Dec i log Msp R25 d Rspot BPTcenter BPTspot
number name (°) (°) (°) (M) (Kpc) (Mpc) (R25)
7977–09102 332.830664 12.184717 41.9 10.935 12.8 251.4 1.0 1 1
8080–09101 47.340029 −0.407944 57.3 9.881 10.5 180.3 1.0 0 0
8244–09101 PGC 25036 133.787581 52.470442 27.4 11.201 18.7 241.6 0.8 0 0
8568–12703 156.810365 38.204502 26.6 10.469 14.5 221.2 0.8 0 0
8716–12703 122.411182 54.552173 43.1 9.770 9.3 174.5 0.7 0 2
8984–12705 NGC 5251 204.353484 27.419218 36.5 11.292 20.3 158.3 0.6 2 0
9031–06104 240.585568 44.470175 41.7 10.019 8.5 185.1 0.9 0 0

Notes. The columns show the MaNGA number, the other name, the right ascension (RA) and the declination (Dec) (J2000.0), the kinematic inclination angle i, the spectroscopic stellar mass Msp in solar masses, the optical radius R25 in kpc, the galaxy distance d in Mpc, the galactocentric distance (normalized to the optical radius R25) of the spot position, the BPT type of the radiation at the center of the galaxy (0 – SF, 1 – intermediate, 2 – AGN), the BPT type of the radiation in the spot of the enhanced gas velocity dispersion.

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