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Table 1

Properties of the 13 LINER 1s showing definite detection of a broad Hα emission (taken from Ho et al. 1997b sample).

Galaxy name RA Dec Hubble type Distancea log(MBH)b
(Mpc) (M)

NGC-266 00 49 47.8 +32 16 40 SB(rs)ab 62.4 8.44
NGC-315 00 57 48.9 +30 21 09 E+: 65.8 9.06
NGC-2681 08 53 32.7 +51 18 49 (R’)SAB(rs)0/a 17.2 6.78
NGC-2787 09 19 18.5 +69 12 12 SB(r)0+ 7.48 8.15
NGC-3226 10 23 27.0 +19 53 55 E2:pec 23.6 8.06
NGC-3718 11 32 34.8 +53 04 05 SB(s)a pec 17.0 7.61
NGC 3998 11 57 56.1 +55 27 13 SA(r)0? 14.1 9.07
NGC 4143 12 09 36.0 +42 32 03 SAB(s)0 15.9 8.18
NGC-4203 12 15 05.0 +33 11 50 SAB0-: 15.1 7.73
NGC-4278 12 20 06.8 +29 16 51 E1+ 16.1 8.72
NGC-4750 12 50 07.2 +72 52 28 (R)SA(rs)ab 26.1 7.27
NGC-4772 12 53 29.1 +02 10 06 SA(s)a 16.3 7.46
NGC-5005 13 10 56.2 +37 03 33 SAB(rs)bc 21.3 7.79

Notes. 

(a)

Distances adapted from Tonry et al. (2001), otherwise from Tully (1988).

(b)

Black hole mass calculated using Graham et al. (2010) updated M − σ relation of Tremaine et al. (2002) with stellar velocity dispersion taken from Ho et al. (2009).

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