80. 90. THE ASTROPHYSICAL JOURNAL, 485 : 434Ã435, 1997 August 10. 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A..
THE ASTROPHYSICAL JOURNAL, 485 : 434È435, 1997 August 10 ( 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
ERRATUM In the paper ““ A Comparison of Radio Axis with Host Galaxy Plane Axis in Seyfert Galaxies ÏÏ by Henrique R. Schmitt, Anne L. Kinney, Thaisa Storchi-Bergmann, & Robert Antonucci (ApJ, 477, 623 [1997]), there are errors in Table 1 and Figure 6, and there is a reference to a previous work that should be stated. With respect to the latter, the authors compare the position angle of small-scale radio structures in Seyfert galaxies with the position angle of their host galaxy major axis. In their analysis they Ðnd a zone of avoidance, where the small-scale radio axis avoids close alignment with the host galaxy minor axis. The authors wish to note that J. S. Ulvestad and A. S. Wilson (ApJ, 285, 439 [1984]) already observed a paucity of radio structures aligned with the host galaxy minor axis in Seyfert 2 galaxies, although on a smaller sample. Ulvestad & Wilson was referenced in their paper as Ulvestad & Wilson (1984b). In Table 1 there were errors in the references listed in the note to the table. A new version of Table 1 with correct references is given here, and the following reference entries should be added to the reference list of the original paper : Mulchaey, J. S., Wilson, A. S., & Tsvetanov, Z. I. 1996, ApJS, 102, 309 ; Oke, J. B., & Lauer, T. R. 1979, ApJ, 230, 360 ; Simkin, S. M. 1975, ApJ, 200, 567. Figure 6a was printed twice, once correctly and once incorrectly in place of Figure 6c. The correct version of Figure 6c appears below.
90
80 70 60 50 40 30 20 10 0
20
40
60
80
FIG. 6.È(c) Results of the Seyfert 2 model. The lines are the cumulative sum of all the vectors with b less than or equal to the value indicated below the line.
434
2 2 2 2 2 2 1.9 1.5 2 1.5 1.5 1.5 2 2 2 1.9 1.9 1.5 2 2 2 2 1.5 2 1 2 1.5 2 1 2 2 1.2 1 2 2 2 2 1 2 2 1 2 2 1 1.5 2
NGC 591 . . . . . . . . . . . . NGC 1068 . . . . . . . . . . . NGC 1144 . . . . . . . . . . . NGC 1386 . . . . . . . . . . . NGC 2110 . . . . . . . . . . . NGC 2273 . . . . . . . . . . . NGC 2992 . . . . . . . . . . . NGC 3227 . . . . . . . . . . . NGC 3362 . . . . . . . . . . . NGC 3516 . . . . . . . . . . . NGC 4051 . . . . . . . . . . . NGC 4151 . . . . . . . . . . . NGC 4117 . . . . . . . . . . . NGC 4388 . . . . . . . . . . . NGC 5135 . . . . . . . . . . . NGC 5252 . . . . . . . . . . . NGC 5273 . . . . . . . . . . . NGC 5548 . . . . . . . . . . . NGC 5643 . . . . . . . . . . . NGC 5728 . . . . . . . . . . . NGC 5929 . . . . . . . . . . . NGC 7172 . . . . . . . . . . . NGC 7450 . . . . . . . . . . . NGC 7672 . . . . . . . . . . . IC 4329A . . . . . . . . . . . . ESO 428[G14 . . . . . . MCG 8-11-11 . . . . . . . Mrk 3 . . . . . . . . . . . . . . . . Mrk 6 . . . . . . . . . . . . . . . . Mrk 34 . . . . . . . . . . . . . . . Mrk 78 . . . . . . . . . . . . . . . Mrk 79 . . . . . . . . . . . . . . . Mrk 110 . . . . . . . . . . . . . Mrk 176 . . . . . . . . . . . . . Mrk 266 . . . . . . . . . . . . . Mrk 268 . . . . . . . . . . . . . Mrk 270 . . . . . . . . . . . . . Mrk 279 . . . . . . . . . . . . . Mrk 348 . . . . . . . . . . . . . Mrk 463E . . . . . . . . . . . . Mrk 509 . . . . . . . . . . . . . Mrk 533 . . . . . . . . . . . . . Mrk 573 . . . . . . . . . . . . . Mrk 618 . . . . . . . . . . . . . Mrk 766 . . . . . . . . . . . . . Mrk 1066 . . . . . . . . . . . .
(RÏ)SB0/a (R)SA(rs)b Ring B SB(s)o SAB0 SB(r)a Sa pec SAB(s)pec SABc (R)SB(s)0 SAB(rs)bc (RÏ)SAB(rs)ab S0 SA(s)b :sp SB(l)ab S0 SA(s)o (RÏ)SA(s)0/a SAB(rs)c (R l)SAB(r)a Sab :pec Sa pec sp (R)SB(r)a Sb SA0 pec SA :(l)0 S S0 SAB0 S S0/E SBb Pair SA(s)0/a pec Compact pec S S0 S0 SA(s)0/a Pair Compact SA(r)bc pec (R)SAB(rs)0 SB(s)b pec (RÏ)SB(s)a (R)SB(s)0
Morphological Type
Distance (Mpc) 62.6 15.3 115.3 9.9 28.7 25.7 28.3 14.4 109.3 36.7 10.2 13.6 12.2 32.8 52.8 91.4 14.9 69.2 14.2 36.5 35.8 35.0 43.7 57.0 62.2 19.0 82.5 55.0 79.3 196.8 150.5 89.1 137.5 109.4 112.6 156.7 37.9 124.3 62.3 202.8 135.1 118.8 68.8 143.1 50.9 49.4
T 0.0 ^ 0.8 3.0 ^ 0.3 ... [0.6 ^ 0.5 [3.0 ^ 0.8 0.5 ^ 0.5 1.0 ^ 0.3 1.0 ^ 0.3 5.0 ^ 0.8 [2.0 ^ 0.4 4.0 ^ 0.3 2.0 ^ 0.3 [2.3 ^ 0.3 3.0 ^ 0.4 2.0 ^ 0.3 [2.0 ^ 0.8 [2.0 ^ 0.3 0.0 ^ 0.4 5.0 ^ 0.3 1.0 ^ 0.4 2.0 ^ 0.7 1.4 ^ 0.5 1.0 ^ 0.8 3.0 ^ 0.9 [0.7 ^ 0.8 [1.6 ^ 0.6 ... [2.0 ^ 1.1 [0.5 ^ 0.6 ... [3.5 ^ 1.5 3.0 ^ 0.8 ... 1.0 ^ 0.9 ... ... [2.0 ^ 1.7 [2.0 ^ 0.4 0.0 ^ 0.4 ... ... 4.0 ^ 0.5 [1.0 ^ 0.5 3.0 ^ 0.9 1.0 ^ 0.6 [1.0 ^ 0.8 7.9 1090.0 29.3 13.0 175.0 19.0 77.0 34.0 2.5 4.3 6.0 125.0 0.6 76.0 58.8 13.5 0.9 15.0 20.0 4.6 24.7 1.8 1.7 1.0 24.0 28.2 71.0 361.0 100.0 6.1 12.0 4.2 2.2 10.4 22.4 17.3 5.7 7.7 480.0 100.0 4.5 66.5 5.5 4.2 15.1 35.5
S 6 cm (mJy) 2 1 9 1 1 1 1 1 9 1 1 1 2 1 2 8 1 6 7 2 1 5 1 2 5 2 4 3 3 3 3 3 3 3 9 3 1 3 3 3 3 9 3 3 3 2
Reference 21.57 22.49 22.67 20.18 22.24 21.18 21.87 20.93 21.55 20.84 19.87 21.44 19.03 22.00 22.29 22.13 19.38 21.94 20.68 20.87 21.58 20.42 20.59 20.59 22.05 21.09 22.76 23.12 22.88 22.45 22.51 21.60 21.70 22.17 22.71 22.71 21.00 22.15 23.35 23.69 22.00 23.05 21.49 22.01 21.67 22.02
log (P ) 6 cm (W Hz~1) [28 28 62 45 1 90 [20 173 57 20 81 77 0 23 25 [10 0 160 87 [53 62 90 100 95 95 129 127 86 177 [22 90 2 88 90 32 70 48 90 170 0 110 117 125 146 16 135
P.A. rad (deg) 11 1 10 13 1 1 1 10 10 12 1 10 2 1 2 10 1 1 7 8 1 5 1 2 5 11 1 1 1 1 1 1 3 3 10 1 1 3 1 1 3 10 1 3 3 11
Reference 5 70 130 25 [18 50 6 155 90 55 135 26 18 92 [5 5 10 125 92 30 45 100 35 50 45 135 180 30 130 27 85 65 50 55 7 95 114 33 111 70 75 147 180 80 66 90
P.A. MA (deg) 14 14 14 14 15 14 1 14 14 10 14 17 14 14 18 15 14 15 18 14 18 14 1 18 14 14 18 15 14 1 1 16 18 18 18 1 15 14 15 10 18 18 18 18 15 14
Reference 33 42 68 20 19 40 26 18 33 35 54 51 18 69 30 15 10 35 5 83 17 10 65 45 50 6 53 56 47 49 5 63 38 35 25 25 66 57 59 70 35 30 55 66 50 45
*P.A. (deg)
40 32 ... 68 40 39 72 48 38 40 41 44 60 77 46 50 27 22 30 55 26 56 31 41 73 55 44 27 51 27 60 46 ... 63 ... 48 25 56 27 ... 25 25 44 39 37 54
i (deg)
NOTE.ÈWe consider Seyfert 1, 1.2, and 1.5 galaxies as Seyfert 1 galaxies and Seyfert 1.8, 1.9, and 2.0 galaxies as Seyfert 2 galaxies. Morphological types were obtained from de Vaucouleurs et al. 1991, except for Mrk 78 (Wilson & Tsvetanov 1994). Col. (12) gives the references for S , P.A. , and P.A. , respectively : (1) Ulvestad & Wilson 1984b ; (2) Ulvestad & Wilson 1989 ; (3) Ulvestad & Wilson 1984a ; rad Morris etMA (4) Ulvestad, Wilson, & Sramek 1981 ; (5) Unger et al. 1987 ; (6) Wilson & Willis 61980 ; (7) al. 1985 ; (8) Wilson & Tsvetanov 1994 ; (9) Edelson 1987 ; (10) Kukula et al. 1995 ; (11) Bower et al. 1995 ; (12) Miyaji, Wilson, & Perez-Fournon 1992 ; (13) Weaver, Wilson, & Baldwin 1991 ; (14) de Vaucouleurs et al. 1991 ; (15) Mulchaey, Wilson, & Tsvetanov 1996 ; (16) Oke & Lauer 1979 ; (17) Simkin 1975 ; (18) This paper.
Type
Name
TABLE 1 SAMPLE PROPERTIES
