Our statistical sample contains 70 galaxies, selected from more than 500 southern spirals with (B-V)T0 (i.e. the total color indexes corrected for differential galactic and internal extinction (to "face-on'') and redshift between B and V bands) in RC3 according to one single criterion: they have distinguishable spiral arms. The mean numerical Hubble stage indexes (T) of these galaixes are from 2 to 6, and ) less than 0.76. D25 and d25, taken from RC3, are the apparent major and minor isophotal diameters measured at or reduced to the surface brightness level -m/ss. It is well known that d25/D25 is usually the approximate value of . Following Peng's method, we have adjusted the value of around in order to do the fitting well, meaning that the inclination of a galaxy may be derived by well-fitting the spiral arms with a logarithmic spiral curve on its image. The resulting inclinations for these galaxies are listed in Table 1 (click here). The errors of our estimation mainly come from: a) the position of starting point for an arm; b) the inclination of a galaxy; c) the position of the galactic center. The errors from the position of the starting point and of the center, however, can be decreased if the grey-scale of an image is modified properly by using IRAF to obtain the fine structure of a galaxy as deeply as we could have. The error estimations are derived from the formulae given by Peng (1988).
PGC | Names | m | T | d | H/D0 | |||||
(') | (Mpc) | (kpc) | ||||||||
PGC 382 | 2 | 5.0 | 54.9 | 5.4738.8% | 20.1 | 0.08826.1% | 137.55 | 3.6026.1% | 0.045 | |
PGC 2052 | NGC 150 | 2 | 3.0 | 66.4 | 17.8727.2% | 6.4 | 0.17726.6% | 21.08 | 1.0826.6% | 0.045 |
PGC 2437 | NGC 210 | 2 | 3.0 | 48.6 | 5.7127.2% | 19.3 | 0.31427.1% | 22.37 | 2.0427.1% | 0.063 |
PGC 2595 | NGC 238 | 2 | 3.1 | 35.6 | 13.8110.7% | 8.2 | 0.12610.2% | 113.91 | 4.1710.2% | 0.063 |
PGC 3089 | NGC 289 | 2 | 4.0 | 50.9 | 7.5630.2% | 14.8 | 0.33829.8% | 21.48 | 2.1129.8% | 0.064 |
PGC 3190 | 4 | 4.2 | 51.9 | 13.4325.1% | 16.6 | 0.06924.4% | 139.99 | 2.8124.4% | 0.053 | |
PGC 5269 | NGC 539 | 2 | 5.0 | 44.7 | 9.4631.9% | 11.9 | 0.11030.7% | 128.80 | 4.1230.7% | 0.069 |
PGC 7379 | NGC 782 | 2 | 3.0 | 29.5 | 9.3219.3% | 12.1 | 0.17218.6% | 78.33 | 3.9218.6% | 0.073 |
PGC 8012 | 2 | 2.6 | 56.5 | 6.5426.3% | 17.0 | 0.16126.1% | 77.45 | 3.6326.1% | 0.102 | |
PGC 8451 | NGC 858 | 2 | 5.0 | 29.4 | 12.919.5% | 8.8 | 0.0688.9% | 164.23 | 3.258.9% | 0.054 |
PGC 9420 | NGC 947 | 2 | 5.2 | 58.3 | 16.0020.2% | 7.1 | 0.09117.8% | 66.31 | 1.7517.8% | 0.043 |
PGC 9426 | NGC 945 | 2 | 4.5 | 33.7 | 9.5624.9% | 11.8 | 0.18822.9% | 59.60 | 3.2622.9% | 0.078 |
PGC 9747 | NGC 986 | 2 | 2.0 | 44.7 | 11.9614.6% | 9.5 | 0.26212.7% | 25.43 | 1.9412.7% | 0.067 |
PGC 9973 | 2 | 3.3 | 59.1 | 10.7721.7% | 10.5 | 0.09417.9% | 115.59 | 3.1617.9% | 0.055 | |
PGC 10336 | NGC 1096 | 2 | 4.2 | 17.3 | 10.7817.7% | 11.5 | 0.09717.9% | 87.16 | 2.5017.9% | 0.050 |
PGC 10870 | 2 | 3.8 | 37.4 | 6.8415.5% | 16.3 | 0.12014.8% | 115.21 | 4.0214.8% | 0.085 | |
PGC 11691 | A0305-31 | 2 | 5.9 | 53.9 | 18.1517.2% | 6.3 | 0.08816.2% | 63.35 | 1.6216.2% | 0.036 |
PGC 12412 | NGC 1300 | 2 | 4.0 | 48.6 | 10.6919.2% | 10.6 | 0.24518.3% | 19.95 | 1.4218.3% | 0.039 |
PGC 13179 | NGC 1365 | 2 | 3.0 | 64.7 | 7.7716.2% | 14.4 | 0.88611.2% | 20.55 | 5.2911.2% | 0.079 |
PGC 13586 | NGC 1433 | 2 | 2.0 | 56.4 | 4.8014.7% | 22.6 | 0.56213.5% | 12.27 | 2.0013.5% | 0.087 |
PGC 14704 | IC 2050 | 2 | 3.0 | 37.4 | 15.2614.9% | 7.5 | 0.05114.6% | 162.65 | 2.4114.6% | 0.048 |
PGC 14897 | NGC 1566 | 2 | 4.0 | 37.4 | 8.3031.8% | 13.6 | 0.29524.6% | 17.60 | 1.5124.6% | 0.035 |
PGC 15850 | NGC 1640 | 2 | 3.0 | 39.1 | 8.1318.9% | 13.8 | 0.19818.5% | 19.71 | 1.1318.5% | 0.075 |
PGC 15941 | NGC 1672 | 2 | 3.0 | 38.7 | 8.804.8% | 12.8 | 0.3704.7% | 15.40 | 1.664.7% | 0.056 |
PGC 16136 | 2 | 4.5 | 43.1 | 9.3329.4% | 12.1 | 0.09537.3% | 76.21 | 2.1137.3% | 0.070 | |
PGC 16751 | A0504-17 | 2 | 5.0 | 52.9 | 10.5624.4% | 10.7 | 0.10819.9% | 58.41 | 1.8319.9% | 0.071 |
PGC 17436 | NGC 1964 | 2 | 3.0 | 74.7 | 10.0521.9% | 11.3 | 0.37817.6% | 20.09 | 2.2117.6% | 0.066 |
PGC 18092 | IC 2160 | 2 | 4.7 | 66.5 | 11.4813.4% | 9.9 | 0.13110.8% | 60.49 | 2.3010.8% | 0.057 |
PGC 19413 | 2 | 3.0 | 70.7 | 16.5429.3% | 6.9 | 0.19125.9% | 31.79 | 1.7725.9% | 0.065 | |
PGC 19498 | 4 | 5.1 | 60.0 | 21.1618.5% | 10.7 | 0.06013.4% | 71.25 | 1.2413.4% | 0.030 | |
PGC 23616 | NGC 2590 | 2 | 3.5 | 76.1 | 8.9335.7% | 12.6 | 0.21035.6% | 64.53 | 3.9435.6% | 0.092 |
PGC 24395 | NGC 2642 | 2 | 4.0 | 21.1 | 8.5120.0% | 13.2 | 0.14019.6% | 55.72 | 2.2719.6% | 0.067 |
PGC 27351 | NGC 2935 | 2 | 3.0 | 50.1 | 9.0723.2% | 12.4 | 0.18518.9% | 27.63 | 1.4918.9% | 0.050 |
PGC 28027 | NGC 3001 | 3 | 3.9 | 47.5 | 10.432.6% | 16.0 | 0.1691.9% | 30.20 | 1.481.9% | 0.052 |
PGC 30108 | NGC 3200 | 2 | 4.5 | 73.0 | 9.2926.5% | 12.2 | 0.30725.5% | 44.33 | 3.9625.5% | 0.070 |
PGC 32026 | NGC 3360 | 4 | 5.0 | 43.6 | 9.8819.2% | 22.1 | 0.07619.2% | 110.28 | 2.4419.2% | 0.063 |
PGC 33919 | 2 | 2.6 | 50.2 | 12.0221.6% | 9.4 | 0.12820.7% | 33.60 | 1.2520.7% | 0.046 | |
PGC 34006 | A1108-09 | 2 | 4.8 | 35.6 | 7.2123.0% | 15.5 | 0.14222.2% | 101.65 | 4.2022.2% | 0.070 |
PGC 42181 | NGC 4575 | 3 | 3.8 | 37.6 | 17.5113.3% | 9.7 | 0.07311.9% | 67.61 | 1.4411.9% | 0.033 |
PGC 45170 | NGC 4939 | 2 | 4.0 | 59.1 | 13.3011.9% | 8.6 | 0.14413.5% | 40.11 | 1.6813.5% | 0.026 |
PGC 45999 | 2 | 2.2 | 74.9 | 8.0724.0% | 13.9 | 0.26322.5% | 44.59 | 3.4122.5% | 0.076 | |
PGC 46974 | NGC 5135 | 2 | 2.0 | 40.9 | 9.5617.3% | 11.8 | 0.22317.3% | 52.79 | 3.4217.3% | 0.087 |
PGC 51456 | NGC 5597 | 2 | 6.0 | 27.4 | 14.836.6% | 7.7 | 0.0906.6% | 33.99 | 0.896.6% | 0.039 |
PGC 53499 | NGC 5792 | 2 | 3.0 | 80.5 | 16.2638.7% | 7.0 | 0.38136.6% | 25.67 | 2.8436.6% | 0.054 |
PGC 54250 | NGC 5833 | 2 | 4.2 | 67.2 | 5.7537.4% | 19.2 | 0.37936.1% | 38.28 | 4.2236.1% | 0.109 |
PGC 55738 | NGC 5968 | 2 | 2.0 | 36.1 | 6.2468.5% | 17.8 | 0.22566.6% | 67.44 | 4.4166.6% | 0.096 |
PGC 56630 | IC 4585 | 2 | 3.0 | 72.4 | 32.1929.1% | 3.6 | 0.07428.4% | 46.64 | 1.0028.4% | 0.028 |
PGC 57924 | NGC 6118 | 2 | 6.0 | 69.7 | 12.6824.4% | 9.0 | 0.26923.4% | 21.63 | 1.6923.4% | 0.052 |
PGC 59325 | IC 4618 | 2 | 4.1 | 50.7 | 9.5819.7% | 11.8 | 0.12814.6% | 38.23 | 1.4214.6% | 0.067 |
PGC 60907 | IC 4664 | 2 | 3.2 | 50.9 | 13.8543.3% | 8.2 | 0.09641.9% | 65.25 | 1.8241.9% | 0.048 |
PGC 61315 | NGC 6492 | 2 | 3.8 | 55.0 | 10.6238.7% | 10.7 | 0.16438.6% | 55.60 | 2.6538.6% | 0.062 |
PGC 63204 | IC 4852 | 2 | 4.5 | 31.7 | 6.8922.6% | 16.2 | 0.15119.1% | 59.64 | 2.6219.1% | 0.093 |
PGC 64042 | IC 4933 | 2 | 4.2 | 31.7 | 15.1210.3% | 7.5 | 0.1219.1% | 64.04 | 2.259.1% | 0.053 |
PGC 64168 | NGC 6862 | 2 | 3.5 | 46.2 | 10.8217.6% | 10.5 | 0.13615.5% | 55.28 | 2.1915.5% | 0.082 |
PGC 64413 | NGC 6872 | 2 | 3.0 | 70.0 | 8.5035.3% | 13.2 | 0.48429.6% | 62.75 | 8.8329.6% | 0.077 |
PGC 65125 | NGC 6937 | 2 | 4.9 | 49.9 | 9.0633.1% | 12.5 | 0.18528.7% | 61.64 | 3.3228.7% | 0.079 |
PGC 67417 | NGC 7125 | 2 | 5.0 | 31.3 | 6.0420.8% | 18.3 | 0.07718.8% | 39.59 | 0.8918.8% | 0.025 |
PGC | Names | m | T | d | H/D0 | |||||
(') | (Mpc) | (kpc) | ||||||||
PGC 67418 | NGC 7126 | 2 | 5.0 | 62.8 | 8.1523.4% | 13.8 | 0.22422.8% | 39.68 | 2.5822.8% | 0.078 |
PGC 67532 | NGC 7141 | 2 | 4.0 | 43.6 | 13.5013.2% | 8.4 | 0.21012.8% | 38.59 | 2.3612.8% | 0.050 |
PGC 69183 | NGC 7309 | 3 | 5.0 | 21.1 | 16.6411.1% | 10.2 | 0.08310.7% | 54.83 | 1.3210.7% | 0.041 |
PGC 69453 | NGC 7329 | 2 | 3.0 | 51.7 | 7.9915.6% | 14.1 | 0.29815.6% | 40.76 | 3.5315.6% | 0.077 |
PGC 69507 | 2 | 5.0 | 30.3 | 16.5912.2% | 6.9 | 0.06111.9% | 144.28 | 2.5611.9% | 0.040 | |
PGC 70027 | NGC 7412 | 2 | 3.0 | 47.9 | 16.3714.2% | 7.0 | 0.19113.6% | 22.67 | 1.2613.6% | 0.049 |
PGC 70096 | NGC 7424 | 2 | 6.0 | 31.7 | 6.597.1% | 16.9 | 0.2159.6% | 12.39 | 0.779.6% | 0.023 |
PGC 70800 | NGC 7531 | 2 | 4.0 | 63.5 | 9.3013.4% | 12.1 | 0.31711.2% | 20.92 | 1.9311.2% | 0.069 |
PGC 70884 | NGC 7552 | 2 | 2.0 | 37.4 | 13.834.9% | 8.2 | 0.2044.9% | 20.91 | 1.244.9% | 0.059 |
PGC 71001 | NGC 7582 | 2 | 2.0 | 63.0 | 12.8616.6% | 8.8 | 0.27816.7% | 20.68 | 1.6716.7% | 0.055 |
PGC 72444 | NGC 7755 | 2 | 4.7 | 45.7 | 6.4516.0% | 17.2 | 0.28815.9% | 39.63 | 3.3215.9% | 0.076 |
PGC 72718 | 2 | 4.7 | 39.5 | 8.9913.1% | 12.5 | 0.11313.1% | 102.64 | 3.3713.1% | 0.088 | |
PGC 72929 | 2 | 3.7 | 46.2 | 8.4018.0% | 13.4 | 0.13516.0% | 63.11 | 2.4816.0% | 0.102 |