The influence of the cluster environment on the large-scale radio continuum emission of 8 Virgo cluster spirals

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Table 2:

Integrated flux densities.
Galaxy name	$S_{\rm TP20~cm}$	$S_{\rm PI20~cm}$	$S_{\rm TP6~cm}$	$S_{\rm PI6~cm}$
	mJy	mJy	mJy	mJy
NGC 4321	$256 \pm 2$	$17.2 \pm 0.5$	$99.1 \pm 0.2$	$14.1 \pm 0.2$
NGC 4388	$178 \pm 2$	-	$81.6 \pm 0.5$	$2.3 \pm 0.1$
NGC 4396	$15.8 \pm 0.5$	$1.5 \pm 0.2$	$8.3 \pm 0.1$	$1.0 \pm 0.1$
NGC 4402	$68 \pm 2$	-	$26.3 \pm 0.2$	$2.5 \pm 0.1$
NGC 4438	$102 \pm 3$	-	$73.9 \pm 0.3$	$6.3 \pm 0.1$
NGC 4501	$331 \pm 2$	$10.4 \pm 0.4$	$96.2 \pm 0.2$	$11.2 \pm 0.1$
NGC 4535	$66 \pm 1$	$13.9 \pm 0.4$	$28.7 \pm 0.2$	$4.2 \pm 0.1$
NGC 4654	$134.6 \pm 0.5$	$6.0 \pm 0.3$	$49.9 \pm 0.1$	$3.1 \pm 0.1$

Source LaTeX | All tables | In the text

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