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Table 3.

Comparison between gas and stellar velocity.

Galaxy vNSC, stars vNSC, gas v2″, stars v2″, gas ⟨log(ΣSFR, NSC)⟩ ⟨log(ΣSFR, 2″)⟩
(km s−1) (km s−1) (km s−1) (km s−1) log(M yr−1 kpc−2) log(M yr−1 kpc−2)
(1) (2) (3) (4) (5) (6) (7)
NGC 853 1534.2 ± 2.0 1552.9 ± 0.7 1528.3 ± 2.2 1542.7 ± 0.4 −0.94 ± 0.12 −1.01 ± 0.40
UGC 3755 316.2 ± 4.8 302.9 ± 0.4 316.7 ± 4.1 305.0 ± 0.5 −1.31 ± 0.17 −1.57 ± 0.31
ESO 59−01 527.2 ± 1.3 524.0 ± 0.5 529.4 ± 3.5 531.9 ± 0.7 −2.09 ± 0.35 −2.52 ± 0.30
IC 1959 645.4 ± 1.3 648.2 ± 0.5 646.0 ± 2.3 647.2 ± 0.4 −1.92 ± 0.21 −1.87 ± 0.46
UGC 5889 568.4 ± 2.0 577.7 ± 2.4 576.2 ± 3.1 568.1 ± 4.4 −2.58 ± 0.85 −3.17 ± 0.10
UGC 8041 1320.6 ± 1.3 1323.2 ± 0.9 1322.1 ± 1.9 1328.1 ± 1.2 −1.15 ± 0.30 −1.79 ± 0.50
NGC 1487 838.0 ± 2.5 851.6 ± 2.0 840.6 ± 3.4 841.6 ± 1.4 −0.34 ± 0.14 −0.62 ± 0.23
NGC 4592 1061.9 ± 1.6 1061.3 ± 0.6 1059.2 ± 1.3 1061.9 ± 0.6 −1.38 ± 0.52 −1.82 ± 0.19
NGC 1796 1015.8 ± 1.4 1019.2 ± 0.3 1017.8 ± 1.0 1012.3 ± 0.4 −0.12 ± 0.43 −1.10 ± 0.41

Notes. (1) Galaxy name, (2), (3) average line-of-sight velocity of the stellar and gaseous component in the NSC spectrum, (4), (5) average line-of-sight velocity of stellar and gaseous components in the circumnuclear spectrum (2″), (6), (7) average SFR density in the NSC (defined by a circular aperture with radius corresponding to the PSF FWHM) and at 2″ (defined by an annular aperture).

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