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

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Volume 512 (March-April 2010)

A&A, 512 (2010) A36

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Table 1:

Integration times and rms.
Galaxy name	$m_{\rm B}$ ¹	i²	Dist.³	Integration	Integration	Bandwidth	Rms TP6 cm	Rms TP20 cm	Rms PI6 cm	Rms PI20 cm
				time (6 cm)	time (20 cm)	(20 cm)	( $\mu$ Jy/	( $\mu$ Jy/	( $\mu$ Jy/	( $\mu$ Jy/
	(mag)	(deg)	(deg)	(h:min)	(h:min)	(MHz)	beam)	beam)	beam)	beam)
NGC 4321	10.02	27^a	4.0	7:45	0:30	$2\times50$	10	110	9	35
NGC 4388	11.87	77^a	1.3	9:25	8:00	VIVA	60	300	9	200
NGC 4396	13.07	72^b	3.5	8:00	0:30	$2\times50$	8	60	9	25
NGC 4402	12.64	74^c	1.4	5:00	8:00	VIVA	21	80	13	100
NGC 4438	11.12	68^a/85^c	1.0	7:45	8:00	VIVA	30	60	14	300
NGC 4501	10.50	57^a	2.0	3:55	5:00	VIVA	14	220	11	50
NGC 4535	10.73	43^a	4.3	9:00	0:30	$2\times50$	9	80	9	35
NGC 4654	11.31	51^a	3.4	7:50	0:30	$2\times50$	9	50	9	30

Notes. ⁽¹⁾ This research has made use of the GOLD Mine Database (Gavazzi et al. 2003); ⁽²⁾ inclination angle; ⁽³⁾ distance from M 87; ^(a) from Cayatte et al. (1990); ^(b) from NED; ^(c) from Kenney et al. (1995).

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