Molecular gas content and SFR in Hickson compact groups: enhanced or deficient?

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Table 3

FIR, SFR, SFE, and sSFR.

Galaxy	Ref.^a	I₆₀	I₁₀₀	log(L_FIR)	SFR	log(SFE)^b	log(sSFR)
		(Jy)	(Jy)	(L_⊙)	(M_⊙ yr^-1)	(yr^-1)	(M_⊙ yr^-1)

7a	2	3.32	6.61	10.23	3.75	–9.14	–10.33
7b	2	<0.18	<0.32	<8.95	<0.20		<–11.30
7c	2	0.61	2.35	9.65	0.99	–9.18	–10.62
7d	2	< 0.15	<0.39	<8.95	<0.20		<–10.63
10a	2	0.50	1.81	9.72	1.16	–9.45	–11.02
....	....	....	....	....	....	....	....

Notes. The full table is available in electronic form at the CDS and from http://amiga.iaa.es.

^(a)

Reference code (see Sect. 3.2): 1: our data analysis. 2: Verdes-Montenegro et al. (1998).

^(b)

The value of the SFE is not displayed for the galaxies with upper limits in both L_FIR and M_H₂.

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