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[vsnet-sequence 43] Nova Suspect in Taurus
Thanks to Arne Henden performing photometry on Didier Favre's nova
suspect in Taurus, I have been able to prepare the following sequence
for this new red variable.
Bruce Sumner
---------------------------
185 Red variable in Taurus (M) Range: unknown
Position: 04 21 12.13 +16 26 17.1 (J2000, Henden astrometry)
Magnitude: V=13.565 BV=1.931 (Henden, 29 Nov 2000)
ID RA (2000) DEC X Y N V ERR BV ERR
a) Comparison star sequence
1 04 21 31.0 +16 23 08 272 189 1 12.363 0.001 1.592 0.002
2 04 20 56.4 +16 24 40 226 97 1 12.871 0.002 1.828 0.004
3 04 21 26.5 +16 31 48 206 331 1 13.082 0.002 1.030 0.003
4 04 20 53.3 +16 24 51 270 86 1 13.677 0.003 1.187 0.004
5 04 21 05.6 +16 21 43 94 274 1 14.317 0.004 1.126 0.006
6 04 20 58.7 +16 24 49 193 88 1 14.633 0.004 1.106 0.006
7 04 21 05.4 +16 29 14 97 177 1 15.251 0.006 1.109 0.009
8 04 21 13.4 +16 25 00 19 77 1 15.969 0.009 0.960 0.013
9 04 21 23.3 +16 25 13 161 64 1 16.529 0.014 1.372 0.030
10 04 21 16.6 +16 25 52 65 25 1 17.388 0.034 1.017 0.051
b) Widecolour extension for CCD calibration
Not required.
Notes:
1. A new red variable star discovered by Didier Favre.
2. A very tentative examination of the available imagery indicates
that this variable has a magnitude range of about 13-20. The
discovery appears to have been made near the time of maximum
magnitude.
3. This is a highly reddened region, and all the stars here are
highly reddened. But it should still be noted that the new red
variable is the reddest object in the immediate vicinity.
Bruce Sumner
30 November 2000
vsnet-adm@kusastro.kyoto-u.ac.jp