Warm dusty discs: exploring the A star 24 μm debris population

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Table 4:

The predicted and measured disc parameters of sources with resolved debris discs in the mid-infrared.
Star		Wavelength	Predicted disc from SED fit		Observed disc		Reference
HD	Name	$\mu$ m	Radius, $^{\prime\prime}$	Flux, mJy	Radius, $^{\prime\prime}$	Flux, mJy
9672	49 Ceti	18	1.42	35	0.98	68	Wahhaj et al. (2007)
32297		18	1.7	80	3.02	80	Moerchen et al. (2007a)
38678	$\zeta$ Lep	18	0.43	475	0.18	400	Moerchen et al. (2007b)
39060	$\beta$ Pic	18	1.59	2688	2.59	4336	Telesco et al. (2005)
109573	HR4796	18	0.51	1307	1.04	807	Telesco et al. (2000)
141569		18	0.45	549	0.63	623	Fisher et al. (2000)
181296	$\eta$ Tel	18	0.53	142	0.5	62	Smith et al. (2009a)
39060	$\beta$ Pic	25	1.24	8005	2.59	6960	Telesco et al. (2005)
172167	Vega	24	14.7	1271	11	1500	Su et al. (2005)
216956	Fomalhaut	24	8.7	939	20	700	Stapelfeldt et al. (2004)

Source LaTeX | All tables | In the text

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