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Table 4

Sample for analysis: radio and optical parameters.

Galaxy V FHI R log W20 HI μ0 r0,pc q rlim / r0 Photometry
(km   s-1) (Jy   km   s-1) (km   s-1) (km   s-1) (km   s-1) Source (mag   arcsec-2) (pc) source
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)

Cam B   78   5.0 32.6   1.65 1.512 H1, H2, H3 21.87 407 0.44 2.40 P1
CGCG 087-33 279   2.6 55.8 1.4 1.746 H1 19.74 532 0.41 4.13 P2
DDO 006 295   3.4 32.9 1.4 1.516 H1 22.04 570 0.29 2.53 P3
DDO 047 272 61.4 111.0     2.06 2.045 H4 21.78 555 1.00 4.20 P4
DDO 099 243 46.0 91.0   2.06 1.958 H4 21.30 393 0.71 2.67 P1
DDO 167 163   4.6 40.2 1.4 1.604 H1 21.65 337 0.60 3.47 P4
DDO 168 191 74.4 88.0   8.24 1.940 H5, H6 20.36 733 0.38 3.96 P1
DDO 181 202 11.4 56.8 1.4 1.754 H1 20.77 356 0.70 2.87 P1
DDO 187 153 12.0 51.4 1.4 1.710 H1 21.71 287 0.60 3.68 P4
DDO 190 151 27.1 64.0   8.24 1.797 H5, H6 19.62 257 0.89 4.21 P1
DDO 226 359   6.1 56.4   1.65 1.750 H7, H3 20.58 982 0.15 3.05 P3
ESO 059-01 530 17.7 104.0   18     2.001 H8 19.84 389 0.80 4.92 P5
ESO 121-20 577 14.1 96.0 18     1.963 H8 20.47 384 0.70 4.48 P5
ESO 137-18 605 37.4 155.0   18     2.183 H8 18.22 727 0.50 6.17 P5
ESO 215-09 597 122.0   93.0 4    1.967 H9 20.90 430 0.83 3.49 P6
ESO 223-09 593 96.2 103.0   8.2 2.009 H10 19.21 1044   0.70 4.35 P7
ESO 269-58 400   7.2 84.0 18     1.899 H11 19.10 636 0.63 4.72 P3
ESO 320-14 654   2.5 61.3 18     1.738 H7 20.26 304 0.70 4.25 P7
ESO 321-14 609   6.4 29.0 1.65 1.459 H8, H3 21.18 522 0.27 2.59 P6
ESO 324-24 526 52.1 113.0   8.2 2.050 H10 20.43 630 0.93 3.13 P6
ESO 325-11 550 25.4 77.0 8.2 1.880 H10 20.93 775 0.35 3.13 P3
ESO 349-31 229   2.7 31.0 8.2 1.453 H10 21.51 323 0.58 3.21 P3
ESO 379-07 644   5.2 40.0   1.65 1.600 H8, H3 22.10 443 0.85 2.81 P6
ESO 381-18 625   3.3 61.6 18     1.741 H7 20.29 224 0.70 4.77 P6, P5
ESO 381-20 596 31.9 103.0   8.2 2.009 H10 20.99 891 0.32 2.89 P8
ESO 384-16 504   1.5 41.0 1.2 1.612 H12 19.45 214 0.92 3.00 P6
ESO 444-78 573   4.0 52.1 1.4 1.716 H1 20.46 475 0.41 3.00 P1
ESO 444-84 583 21.1 75.0 4    1.873 H8, H13 20.60 318 0.89 2.46 P1
ESO 461-36 427   7.5 84.0 10.2   1.916 H7, H14 20.51 492 0.50 4.58 P7
GR 8 214   7.8 39.2 1.4 1.592 H1 21.36 152 0.80 3.70 P4
Ho II 156 267.0   72.0 5.2 1.854 H15 19.66 1348   1.00 2.25 P9
IC 3104 429 10.3 63.0 18     1.753 H8 18.85 468 0.45 3.42 P3
IC 4247 419   3.4 49.0 18     1.608 H16 18.77 370 0.33 5.30 P2, P5
IC 4316 576   2.1 32.8   1.65 1.513 H16, H3 20.31 520 0.60 4.47 P5
IC 4662 302 130.0   133.0   18     2.114 H8 17.40 242 0.73 5.69 P3
IC 5152 122 97.2 100.0   18     1.983 H8 18.08 345 0.66 5.22 P3
KK98 17 156   1.0 53.0 10.2   1.705 H14 21.67 470 0.31 2.98 P10
KK98 182 613   2.1 24.0 7.9 1.316 H14 21.28 400 0.68 3.07 P3
KK98 200 494   1.7 26.5   1.65 1.421 H1, H3 20.51 179 0.70 5.17 P7
KK98 230   63   2.6 25.9   1.65 1.411 H1, H17 22.57 140 0.95 1.76 P11
KKH 086 287   0.5 20.6 1.4 1.310 H1 21.56 181 0.61 1.98 P3
KKH 098  −132   4.1 31.5   1.65 1.498 H1, H3 21.39 184 0.59 2.68 P10
Mrk 178 250   3.0 44.8 1.4 1.650 H1 19.15 228 0.50 5.56 P4
NGC 1311 568 14.6 105.0   18     2.005 H8 19.15 586 0.40 5.36 P12
NGC 1569  −86 84.0 123.8   5.2 2.092 H18 16.83 271 0.55 6.13 P4
NGC 2915 468 145.0   163.0   6.6 2.211 H19 17.49 306 0.50 7.67 P5
NGC 3077  −20 256.0   157.3   5.2 2.196 H18 17.28 593 0.70 4.50 P9
NGC 3738 225 22.0 122.0     8.24 2.084 H6 18.41 437 0.70 5.08 P4
NGC 4163 164   9.6 38.0 4.1 1.574 H5, H20 19.29 223 0.70 5.18 P4
NGC 4214 293 319.8   89.8 2.6 1.952 H5, H18 17.63 491 0.50 4.46 P9
NGC 5408 506 65.5 123.0   8.2 2.087 H10 18.88 456 0.50 7.03 P5
NGC 6822  −55 2266.0     115.0   1.9 2.061 H21, H22 19.55 239 0.80 1.87 P9
Peg DIG  −183   28.1 38.6 5.3 1.577 H23 20.93 333 0.55 2.08 P10
Sex A 324 168.0   64.0   1.12 1.806 H24 21.09 362 0.95 3.03 P3
Sex B 301 72.9 56.0 1.4 1.747 H1 20.57 255 0.87 3.53 P6
UGC 0685 156 13.4 83.0   1.65 1.919 H25, H3 19.72 336 0.70 5.07 P12
UGC 3755 315   6.8 50.6   1.4 1.703 H1 19.81 808 0.50 3.72 P2
UGC 4115 343 21.0 106.0     1.65 2.025 H5, H3 20.24 803 0.40 3.74 P4
UGC 4483 156 13.6 50.6 1.4 1.703 H1 20.70 306 0.55 2.81 P1
UGC 6456  −94 10.1 52.0   1.65 1.716 H3 20.16 248 0.70 5.08 P4
UGC 7605 310   5.7 43.7 1.4 1.640 H1 20.75 402 0.67 3.91 P11
UGC 8508   56 18.3 65.0   1.65 1.813 H3 19.95 234 0.55 4.64 P13
UGC 8833 227   6.0 42.8 1.4 1.631 H1 20.94 274 0.77 4.05 P2
UGCA 092  −95 104.7   73.0   1.65 1.863 H5, H3 20.53 635 0.50 2.40 P4
UGCA 438 62 15.0 35.0 8.2 1.514 H26 20.48 283 0.90 3.97 P3
WLM  −122     292.0   81.0   1.12 1.909 H24 21.28 437 0.40 3.06 P7

Notes. (1) Name of galaxy; (2) heliocentric radial velocity defined by HI; (3) integrated HI flux; (4) apparent full width of 21 cm line at 20% of peak; (5) FWHM of instrumental profile; (6) logarithm of the 21 cm line width at 20% of peak, corrected for instrumental broadening and redshift; (7) source of HI data; (8) central surface brightness of sech model, corrected for extinction and redshift; (9) scale length of sech model in parsecs; (10) adopted ratio of minor to major axes of isophotes; (11) ratio of radius of limiting isophote to scale length of sech; (12) source of surface photometry.

References. (H1) Huchtmeier et al. (2003); (H2) Begum et al. (2003); (H3) Begum et al. (2008); (H4) Springob et al. (2005); (H5) Huchtmeier & Richter (1986); (H6) Stil & Israel (2002); (H7) Meyer et al. (2004); (H8) Koribalski et al. (2004); (H9) Warren et al. (2004); (H10) Cote et al. (1997); (H11) Banks et al. (1999); (H12) Beaulieu et al. (2006); (H13) de Blok et al. (2002); (H14) Huchtmeier et al. (2000); (H15) Bureau & Carignan (2002); (H16) Minchin et al. (2003); (H17) Begum et al. (2006); (H18) Walter et al. (2008); (H19) Meurer et al. (1996); (H20) Swaters et al. (2002); (H21) de Blok & Walter (2006); (H22) Weldrake et al. (2003); (H23) Kniazev et al. (2009); (H24) Barnes & de Blok (2004); (H25) Giovanelli & Haynes (1993); (H26) Longmore et al. (1978); (P1) CFHT 2004: Fingerhut et al. (2010); (P2) SPM 2005: Fingerhut et al. (2010); (P3) IRSF 2006: Fingerhut et al. (2010); (P4) CFHT 2002: Vaduvescu et al. (2005); (P5) CTIO 2008: this paper; (P6) IRSF 2005: Fingerhut et al. (2010); (P7) CTIO 2007: Vaduvescu & McCall (2008); (P8) CTIO 2006: Fingerhut et al. (2010); (P9) 2MASS: Vaduvescu & McCall (2008); (P10) CFHT 2005: Fingerhut et al. (2010); (P11) CFHT 2006: Fingerhut et al. (2010); (P12) ESO 2008: this paper; (P13) SPM 2002: Vaduvescu et al. (2005).

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