A mid-IR study of Hickson compact groups - I. Probing the effects of environment in galaxy interactions

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Table 3:

Observed and predicted IRAS $60~\mu$ m and 100 $\mu$ m fluxes.
HCG	IRAS $60~\mu$ m		IRAS $100~\mu$ m
group	Observed	Predicted	Observed	Predicted
	mJy	mJy	mJy	mJy
19	300	246.8	1110	673
26	540	450.6	1496	976
33	<660	339.6	<1140	752
37	$\sim$ 560	449.5	<2000	665
38	$\sim$ 1430	1439	<3160	2076
40	<1090	1478	3850	3686
47	<580	880.9	<1510	1336
54	300	278.2	710	675
55	200	139.4	1630	322
56	<690	1860	<1510	2637
57	<460	437.5	<1380	917
71	1640	736.9	<3070	1069
79	$\sim$ 960	584.4	<2320	1137
95	941	616.2	2390	898

Source LaTeX | All tables | In the text

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