A Herschel PACS and SPIRE study of the dust content of the Cassiopeia A supernova remnant

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Table 1:

Total and individual component flux densities (in Jy) for Cas A.
	70 $\mu$ m	100 $\mu$ m	160 $\mu$ m	250 $\mu$ m	350 $\mu$ m	500 $\mu$ m
Published	107¹	105²	101²	76³	49³	42³, 70⁴
	$\pm$ 22	$\pm$ 21	$\pm$ 20	$\pm$ 16	$\pm$ 10	$\pm$ 8, $\pm$ 16
Herschel	169	192	166	168	92	52
	$\pm$ 17	$\pm$ 19	$\pm$ 17	$\pm$ 17	$\pm$ 10	$\pm$ 7
Nonthermal	6.3	8.1	11.2	15.4	19.4	24.9
	$\pm$ 0.6	$\pm$ 0.7	$\pm$ 0.9	$\pm$ 1.1	$\pm$ 1.3	$\pm$ 1.6
Warm dust	120	63	22	7.0	3.1	1.2
	$\pm$ 12	$\pm$ 6	$\pm$ 2	$\pm$ 0.8	$\pm$ 0.4	$\pm$ 0.2
Cold IS dust	18	76	123	141	69	27.5
	$\pm$ 4	$\pm$ 11	$\pm$ 17	$\pm$ 17	$\pm$ 10	$\pm$ 7
Cool dust	25	29⁵	10	4.6	0.5	-1.6
	$\pm$ 7	$\pm$ 11	$\pm$ 17	$\pm$ 17	$\pm$ 10	$\pm$ 4

Notes. ⁽¹⁾ MIPS (Hines et al. 2004); ⁽²⁾ AKARI 90 and 170 $\mu$ m (Sibthorpe et al. 2010); ⁽³⁾ BLAST 250, 350 and 500 $\mu$ m (Sibthorpe et al. 2010); ⁽⁴⁾ SCUBA 450 $\mu$ m (Dunne et al. 2003); ⁽⁵⁾ after subtracting a line contribution of 16 Jy (see Sect. 3).

Source LaTeX | All tables | In the text

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