[vsnet-alert 4053] TmzV85 sequence

["Bruce Sumner" <b.sumner@bom.gov.au>]

Here is a preliminary sequence for this variable, based on field 
photometry obtained by Arne Henden.

     TmzV85   (UG)   Range: 13.517.9V
     Position:   10 43 56.8  +58 07 33    (J2000, from .dat file)
     Magnitude:  V=17.906   V=0.191       (in .dat file)
                                                            
ID      RA  (2000)  DEC       X    Y  N    V      ERR     BV    ERR 

1   10 44 38.6  +58 03 33   332 240  2  12.292  0.006   0.850  0.005 
2   10 43 32.9  +58 11 43  189  249  2  13.262  0.006   0.213  0.004 
3   10 43 44.4  +58 06 08   98  85  2  13.556  0.006   0.919  0.006 
4   10 44 34.7  +58 08 22   300   49  2  14.245  0.000   0.840  0.007 
5   10 44 38.7  +58 08 23   332   50  2  14.667  0.006   0.797  0.003 
6   10 43 38.4  +58 09 15  145  102  2  15.582  0.008   0.576  0.006 
7   10 44 21.4  +58 02 56   195 277  2  16.548  0.000   0.532  0.011 
8   10 44 18.9  +58 04 18   175 195  2  17.166  0.023   0.569  0.045 
9   10 43 54.3  +58 07 11   20  22  2  17.633  0.037   1.145  0.027 
10  10 44 04.3  +58 07 43    59   10  2  17.844  0.016   0.620  0.136 
11  10 43 28.5  +58 05 43  224 110  2  18.607  0.033   0.345  0.120 

Notes:

The position of the variable has not been uniquely determined, the 
position quoted here is the average position of a double star 
separated a just a few arcsecs. The variable could be either the 
fainter northern component or the slightly brighter southern 
component. Similarly the quiescent magnitude quoted above is the 
combined magnitude of the two stars. Also note the large errors in 
the B-V values of the two faintest comparison stars - they are 
unacceptably large.

Bruce Sumner
20 January 2000

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