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[vsnet-obs 21035] Re: V382 Vel comp stars 56 &59
- Date: Tue, 8 Jun 1999 10:09:00 +1000
- To: vsnet-obs@kusastro.kyoto-u.ac.jp, Berto Monard <LAGMonar@csir.co.za>
- From: "Bruce Sumner" <b.sumner@bom.gov.au>
- Subject: [vsnet-obs 21035] Re: V382 Vel comp stars 56 &59
- In-reply-to: <s75b8b1f.085@csir.co.za>
- Priority: normal
- Reply-to: b.sumner@bom.gov.au
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
In reply to Berto's observation that on the V382 Vel chart
comparison star 59 appeared brighter than 56.
This observation nicely shows the pitfalls that bedevil a good
variable star sequence. Both magnitudes are taken from Tycho, and are
accurate, but....
Here are the the V, B-V and derived v(visual) values for these two
stars. v is derived from v=V+0.2*(B-V)
V B-V v Comment
5.56 1.56 5.87 very red
5.90 0.17 5.93 =IW Vel, a low amplitude blue variable
59=IW Vel apparently has an amplitude of about 0.02B, and a period
of 0.14 days. This low amplitude should not preclude it from being
used as a comparison star, but if possible no known variable should
be used as a comparison star.
56 is a red star, and visually will appear fainter, how much depends
on the individual observer. It does not make a good comparison star.
Thus Berto's observation that 59 appeared brighter than 56 is very
plausible. The moral of this tale - comparison stars should not be
variable stars and always try to use comparison stars with silmilar
colours, i.e. don't mix red and blue stars in the same sequence.
Bruce Sumner
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