Herschel photometry of brightest cluster galaxies in cooling flow clusters

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Table 2:

Summary of results and other cluster properties.
Cluster	A1068	A2597	Zw3146
Dust Temperatures	24 $\pm$ 4 K	21 $\pm$ 6 K	23 $\pm$ 5 K
	57 ⁺¹²_-4 K	48 ⁺¹⁷_-5 K	53 ⁺²²_-6 K
Cold Dust Mass	$5.1\times 10^{8}~M_\odot$	$2.3\times 10^{7}~M_\odot$	$5.4\times 10^{8}~M_\odot$
Warm Dust Mass	$3.9\times 10^{6}~M_\odot$	$2.9\times 10^{5}~M_\odot$	$1.9\times 10^{6}~M_\odot$
Total FIR Luminosity	$3.5\times 10^{11}~L_\odot$	$8.8\times 10^{9}~L_\odot$	$2.5\times 10^{11}~L_\odot$
Star Formation Rate	$60\pm 20~M_\odot$ yr^-1	$2\pm 1~M_\odot$ yr^-1	$44 \pm 14~M_\odot$ yr^-1
SFR Spitzer	188 $M_\odot$ yr^-1	4 $M_\odot$ yr^-1	70 $\pm$ 14 $M_\odot$ yr^-1
SFR optical/UV	20-70 $M_\odot$ yr^-1	10-15 $M_\odot$ yr^-1	47 $\pm$ 5 $M_\odot$ yr^-1
CO gas mass	$4.1\times 10^{10}~M_\odot$	$2.0\times 10^{9}~M_\odot$	$7.7\times 10^{10}~M_\odot$
H $\alpha$ Slit Luminosity	$8\times 10^{41}$ erg s^-1	$3\times 10^{41}$ erg s^-1	$3\times 10^{42}$ erg s^-1

Notes. The Spitzer SFR values are from O'Dea et al. (2008), Donahue et al. (2007) and Egami et al. (2006). The Optical/UV SFR values are from McNamara et al. (2004), Donahue et al. (2007) and Egami et al. (2006). The CO gas masses are from Edge (2001) and Salomé (priv. comm.) and the H $\alpha$ slit luminosities are from Crawford et al. (1999).

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