[vsnet-alert 5829] Re: New Haseda variable (HadV82) = WR104

[Brian Skiff <bas@lowell.edu>]

     These stars, extracted from my photometric reference file, are
probably isloated enough from nebulosity to serve for calibration on 
wide-field images for WR 104 (and to provide true V calibration):

Name              RA   (2000)   Dec     s    GSC       V     B-V
NGC 6514 291   18 03 07.8   -23 05 50   G 6842-0020  10.23   0.06
NGC 6514 331   18 03 18.6   -23 10 44   G 6842-1378  11.02   0.11
NGC 6514 163   18 02 30.7   -23 09 06   G 6842-0599  11.64  -0.10
NGC 6514 196   18 02 32.9   -23 06 31   G 6842-0593  12.29   0.15
NGC 6514 160   18 02 29.9   -23 07 47   G 6842-0369  12.65   0.64
NGC 6514 157   18 02 26.9   -23 05 42   G 6842-0060  13.15   0.56


\Brian

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