Table 4.
Properties of GRGs taken from literature.
Name | Re | SFR | log M(H2) | log M* | log L22 μm | FWHM | Refs. |
---|---|---|---|---|---|---|---|
(kpc) | (M⊙ yr−1) | (M⊙) | (M⊙) | (erg s−1) | (km s−1) | ||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
NGC315 | 6.3 | 0.63 | 7.87 | 11.49 | 42.18 | 150 | (1) |
3C31 | 4.6 | 1.02 | 9.22 | 11.29 | 41.51 | 550 | (1) |
3C236 | 7.4 | 7.51 | 9.32 | 11.15 | 43.07 | – | (2) |
3C326N | 6.9 | 0.67 | 9.18 | 11.40 | 42.09 | 351 | (3) |
Notes. Column 2 lists the half-light radius (Re), Col. 3 the star formation rate (SFR), Col. 4 the molecular mass (log M(H2)), Col. 5 the stellar mass (log M*), Col. 6 the 22 μm luminosity derived from WISE (log L22 μm), and Col. 7 the CO(1-0) line width (FWHM) obtained from the respective references listed in Col. 8.
References. (1) Ocaña Flaquer et al. (2010); (2) Labiano et al. (2013); (3) Nesvadba et al. (2010).
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