Table 1
The source list of the 21 galaxies observed for HC3N emission using the Effelsberg 100m and the SMT telescope.
Galaxy | RA (J2000) Dec | VHelio | Distance | log LIR | ΔVCO | Telescope | |
h m s | ° ′ ′′ | (km s-1) | (Mpc) | (L⊙) | (km s-1) | ||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|||||||
NGC 520 | 01 24 34.9 | +03 47 30.0 | 2281 | 30.22 | 10.91 | 270 | Effelsberg |
NGC 660 | 01 43 02.4 | +13 38 42.0 | 850 | 12.33 | 10.49 | 280 | Effelsberg |
NGC 891 | 02 22 33.4 | +42 20 57.0 | 528 | 8.57 | 10.27 | 110 | Effelsberg |
NGC 972 | 02 34 13.4 | +29 18 41.0 | 1543 | 20.65 | 10.67 | 220 | Effelsberg |
NGC 1068 | 02 42 41.4 | −00 00 45.0 | 1137 | 13.7 | 11.27 | 280 | Effelsberg & SMT |
IC 342 | 03 46 48.5 | +68 05 46.0 | 31 | 4.60 | 10.17 | 72.8a | Effelsberg & SMT |
UGC 2855 | 03 48 20.7 | +70 07 58.0 | 1200 | 19.46 | 10.75 | ... | Effelsberg |
UGC 2866 | 03 50 14.9 | +70 05 40.9 | 1232 | 20.06 | 10.68 | ... | Effelsberg |
NGC 1569 | 04 30 49.0 | +64 50 53.0 | −104 | 4.60 | 9.49 | 90 | Effelsberg |
NGC 2146 | 06 18 39.8 | +78 21 25.0 | 882 | 16.47 | 11.07 | 320 | Effelsberg & SMT |
NGC 2403 | 07 36 51.3 | +65 36 29.9 | 161 | 3.22 | 9.19 | 90 | Effelsberg |
M 82 | 09 55 53.1 | +69 40 41.0 | 187 | 3.63 | 10.77 | 150 | Effelsberg & SMT |
NGC 3079 | 10 01 57.8 | +55 40 47.0 | 1116 | 18.19 | 10.73 | 380 | Effelsberg |
NGC 3310 | 10 38 45.9 | +53 30 12.0 | 993 | 19.81 | 10.61 | 140 | Effelsberg |
M 66 | 11 20 15.0 | +12 59 30.0 | 727 | 10.04 | 10.38 | 180 | Effelsberg |
IC 694 | 11 28 33.8 | +58 33 45.0 | 3120 | 47.74 | 11.63 | 250 | Effelsbergb & SMT |
NGC 3690 | 11 28 30.8 | +58 33 43.0 | 3120 | 47.74 | 11.32 | 260 | Effelsbergb & SMT |
Mrk 231 | 12 56 14.2 | +56 52 25.0 | 12600 | 171.84 | 12.51 | 167 | Effelsberg |
Arp 220 | 15 34 57.1 | +23 30 10.0 | 5352 | 79.90 | 12.21 | 360 | Effelsberg & SMT |
NGC 6240 | 16 52 58.9 | +02 24 03.0 | 7160 | 103.86 | 11.85 | 420 | SMT |
NGC 6946 | 20 34 52.6 | +60 09 12.0 | 53 | 5.32 | 10.16 | 130 | Effelsberg & SMT |
Notes. The columns are: (1) galaxy name; (2) and (3) coordinates; (4) heliocentric velocities; (5) distances; (6) total infrared luminosities (from Sanders et al. 2003); (7) CO 1−0 line width (FWHM) of the galaxies; and (8) the telescope these galaxies were observed with.
For IC 342, the ΔV is of CO 2−1 from Gao & Solomon (2004a); for other galaxies ΔV are of CO 1−0 from Young et al. (1995).
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