Table 1: The integrated flux density of OA 184 at four radio frequencies. All values are calculated for this paper from original data. Fluxes of small diameter sources and the synchrotron ridge that the object sits atop (Leahy & Tian 2005) were removed prior to the integration of the continuum brightness temperature. The 151 MHz flux density is an upper limit (see text).
$\nu$ S

(MHz) (Jy)

151 $13.7\pm 3.0$

408 $9.9\pm 1.3$

1420 $8.2\pm 1.0$

2695 $7.7\pm1.0$

4800 $5.7\pm 0.8$

**Table 1:** The integrated flux density of OA 184 at four radio frequencies. All values are calculated for this paper from original data. Fluxes of small diameter sources and the synchrotron ridge that the object sits atop (Leahy & Tian 2005) were removed prior to the integration of the continuum brightness temperature. The 151 MHz flux density is an upper limit (see text).
$\nu$	S
(MHz)	(Jy)
151	$13.7\pm 3.0$
408	$9.9\pm 1.3$
1420	$8.2\pm 1.0$
2695	$7.7\pm1.0$
4800	$5.7\pm 0.8$

Source LaTeX | All tables | In the text