While working through a list of old, but still poorly identified southern variables (announced in Union Obs. Circ. 48 (1920)), I had a bit of trouble with the Mira variable TZ Velorum. The discovery note says that it is the "middle star of three, others 12.5 (mag)". My Guide8 display shows no such configuration, so the GCVS position was probably off. TZ Vel did not appear to be in the GSC, nor did it show up on various photos I checked. Finally I found a bright star in the USNO-A2.0 cat., about 10s of RA to the east. Its mags. are r = 8.6. b = 13.3, V =104, position 9:30:27.35 -53:8:47.2. This must be be TZ Vel, but where were the 12.5 mag companions? A look at the DSS image soon made things clear. 1). The companions are GSC 8584-01180 (13.0) and 8584-4631 (13.8), separation about 20", and somewhat fainter than expected. There is a faint star halfway between them. 2). The USNO-A2.0 position (above) is slightly off, probably skewed by one or more companions just to the east. Checking the GSC 2.2 catalogue turned up the position of the faint star referred to in 1). Its photometry is R = 16.19, B = 18.05 (yielding an approx. V =16.9). I take this to be TZ Vel, position 9:30:26.71 -53:8:46.3 (2000), in very good agreement with the note in UOC48. As a matter of interest, TZ Vel was picked and followed by Vello Tabur. His uncalibrated light curve can be found at http://vsnet.tip.net.au/~vello/varstar The small scale of his images (50"/pixel) are not suited for determining accurate positions, but his light curve suggests a period of about 370d, rather than 237.4d. Regards, Mati Morel morel@ozemail.com.au