Table 4: Derived parameters of the observed sources. Optical line luminosities are from Crawford et al. (1999). Mass deposition rates and cooling radius are from (1) Peres et al. (1998) and (2) White et al. (1997). Dust masses are evaluated from 60 $\mu $m data compiled in Edge (2001), assuming $T_{\rm dust}=35$ K.
Source $M({\rm H}_2)$ $M_{\rm dust}$ L(H$_{\alpha }$) $\dot{M}^{(1)}$ $r_{\rm cool}^{(1)}$ $\dot{M}^{(2)}$ $r_{\rm cool}^{(2)}$ Flux (1.4 GHz)
  ($M_\odot$) ($M_\odot$) (erg/s) ($M_\odot$/yr) (kpc) ($M_\odot$/yr) (kpc) (m Jy)
A262 $2.3\pm0.3\times10^8$ $8.7\times10^6$ $6.0\times10^{39}$ 27 104 10 67 131
pks 0745-191 $4.0\pm0.9\times10^{9}$ $3.5\times10^7$ $1.4\times10^{42}$ 1038 214 579 177 2370
rx j0821+07 $1.3\pm0.2\times10^{10}$ $4.2\times10^7$ $3.0\times10^{41}$ - - - - -
A1068 $4.2\pm0.2\times10^{10}$ $1.4\times10^8$ $1.7\times10^{42}$ - - - - -
A1795 $4.8\pm0.6\times10^9$ $6.7\times10^7$ $1.1\times10^{41}$ 381 177 321 181 930
Z8193 $1.5\pm0.3\times10^{10}$ $3.8\times10^7$ $1.5\times10^{42}$ - - - - -
A496 $4.3\pm1.0\times10^{8}$ - $3.4\times10^{42}$ 95 110 134 138 -
A646 $7.9\pm0.2\times10^{9}$ $2.5\times10^7$ $1.6\times10^{41}$ - - - - -
A780 $2.0\pm0.3\times10^9$ $3.0\times10^7$ $1.6\times10^{41}$ 262 162 222 170 40800
A2657 $2.9\pm0.1\times10^8$ - - - - 44 101 -
A85 $\le$ $8.8\times10^{8}$ - - 107 93 108 131 58
Z235 $\le$ $2.5\times10^{9}$ - - - - - - -
A291 $\le$ $1.1\times10^{10}$ $84.9\times10^7$ $4.6\times10^{41}$ - - - - -
A644 $\le$ $1.1\times10^{9}$ - - 189 141 136 111 -
rx j0439+05 $\le$ $9.8\times10^{9}$ $5.1\times10^7$ $1.1\times10^{42} $ - - - - -
A978 $\le$ $9.3\times10^{8}$ - $2.0\times10^{40}$ - - - - -
A1668 $\le$ $1.5\times10^{9}$ - $1.2 \times10^{41}$ - - - - -
A2029 $\le$ $1.7\times10^{9}$ - $8.0\times10^{39}$ 555 186 431 192 550
MKW3s $\le$ $5.2\times10^{8}$ - $5.0\times10^{39}$ 175 171 132 158 -
A2146 $\le$ $8.6\times10^{9}$ $8.8\times10^7$ $1.4\times10^{42}$ - - - - -
A2142 $\le$ $1.8\times10^{9}$ - - 350 150 369 172 -
A2147 $\le$ $4.3\times10^{8}$ - $7.0\times10^{39}$ - - - - -
A2151 $\le$ $3.1\times10^{8}$ - $5.8\times10^{40}$ - - 166 146 -
A2199 $\le$ $2.6\times10^{8}$ - $3.5\times10^{40}$ 154 143 97 124 3700
A2261 $\le$ $1.3\times10^{10}$ - - - 20 53 - -
A2319 $\le$ $6.6\times10^{8}$ - $1.0\times10^{41}$ - - - - -
CygA $\le$ $1.4\times10^{9}$ - $6.5\times10^{42}$ 244 135 242 167 -
A2462 $\le$ $1.6\times10^{9}$ - $5.8\times10^{40}$ - - - - -
A2597 $\le$ $1.8\times10^{9}$ $8.4\times10^7$ $5.2\times10^{41}$ 271 152 - - 1880
A2626 $\le$ $7.6\times10^{8}$ - $3.3\times10^{40}$ - - 53 114 -
A2634 $\le$ $3.2\times10^{8}$ - $3.7\times10^{40}$ - - - - 7657
A2665 $\le$ $7.9\times10^{8}$ - $6.0\times10^{39}$ - - - - -


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