Table 2: Radio continuum results.
Object $S_{\rm 3~cm}$ $S_{\rm 6~cm}$ RA, Dec (J2000) $\alpha$

(mJy) (mJy) (hms, dms)

WR 21a <0.3 $0.25\pm0.06$ 10:25:56.49 -57:48:43.3 <0.3

S2 $0.55\pm0.10$ $0.36\pm0.06$ 10:25:56.49 -57:48:34.4 0.72

**Table 2:** Radio continuum results.
Object	$S_{\rm 3~cm}$	$S_{\rm 6~cm}$	RA, Dec (J2000)	$\alpha$
	(mJy)	(mJy)	(hms, dms)
WR 21a	<0.3	$0.25\pm0.06$	10:25:56.49 -57:48:43.3	<0.3
S2	$0.55\pm0.10$	$0.36\pm0.06$	10:25:56.49 -57:48:34.4	0.72

Source LaTeX | All tables | In the text

	1 Introduction
	2 WR 21a and its surroundings
	3 Observations and data reduction
	4 Results
	5 Analysis of the line features
	6 The X-ray history of WR 21a
	7 Connection with the EGRET source?
	8 Summary and conclusions
	References