> I'm wondering which stars are being used as comparisons for > Omega CMa? Southern CMa seems to be littered with bright > low-amplitude variables, so I had considered including this > region in BVfSO. But I gave up, frustrated by the apparent > shortage of suitable comparison stars. > > So what comparisons are the various Omega CMa observers > using? > > I had a quick eyeball of Omega CMa last night and earlier > tonight, and both times it looked to be of equal magnitude > to Delta Col (3.85V). > > Hi, Fraser: Although most of the stars in the region are slightly variable I use to make two or three estimates with different comparison stars to eliminate possible errors and there has been no problem. Omega CMa is at 3.9 and the comparison stars I use are: k Puppis, a Be variable with near 0.05 mag. of amplitude. V= 3.82, B-V= -0.16 3 Puppis, an A supergiant only suspected to vary in V. V= 3.96, B-V= 0.18 and 11 Puppis, an F8 bright giant. V= 4.20, B-V= 0.72. Delta Col V= 3.84, B-V= 0.86 is a little too far away and too orange. k Pup is the best one for position and color. Anyway I think omega CMa should be included in a new version of BVfSO called NEVfSO, you know why...:-) Cheers, Sebastian. --- Outgoing mail is certified Virus Free. Checked by AVG anti-virus system (http://vsnet.grisoft.com). Version: 6.0.237 / Virus Database: 115 - Release Date: 07/03/01