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Table 4.

Parameters of LTGs with a disc break.

Object Br σnBr μBr hin
hout
Break type Hubble type (T)
[arcsec] [kpc] [arcsec] [] [arcsec] g − i [mag] [arcsec] g − i [mag]
(1) (2) (3) (4) (5) (6) (7) (8)
FCC013(NGC 1310) 76.8 7.76 3.7 25.01 54.2 0.83 ± 0.03 43.7 1.27 ± 0.1 III 5
FCC022(NGC 1317) I 1
FCC028 38.8 3.91 1.6 23.60 24.0 0.83 ± 0.1 60.8 0.87 ± 0.1 III 9
FCC029(NGC 1326) 53.6 5.41 1.5 21.82 24.76 0.92 ± 0.07 159.8 0.68 ± 0.03 III 1
FCC033(NGC 1316C) I 7
FCC035 27.6 2.8 0.3 23.94 25.64 −0.57 ± 0.02 34.2 −0.93 ± 0.1 III 9
FCC037(NGC 1326A) I 5
FCC039(NGC 1326B) 95.5 9.64 8.2 25.01 94.9 0.52± 0.02 37.0 0.88 ± 0.2 III 7
FCC062(NGC 1341) 52.3 5.28 2.3 24.03 38.9 0.78 ± 0.02 68.2 0.86 ± 0.03 III 4

Notes. Column 1 – LTGs with a disc break; Col. 2 – Break radius in units of arcsec and kpc (1 arcsec = 0.101 kpc); Col. 3 – Standard deviation of the break radii from (n + 1)3 combinations; Col. 4 – Surface brightness at the break radius; Col. 5 – Inner scale-length in units of arcsec, and average g − i colour for hin; Col. 6 – Outer scale-length in units of arcsec, and average g − i colour for hout; Col. 7 – Profile classification; Col. 8 – Hubble type T taken from Drinkwater et al. (2001b).

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