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[vsnet-chat 1340] Re: Designation of new variable stars
- Date: Sun, 27 Sep 1998 09:05:53 -0700
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: aah@nofs.navy.mil
- Subject: [vsnet-chat 1340] Re: Designation of new variable stars
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Brian and Taichi have given a good dialog on variable star designations. While Brian feels
6arcsec resolution is sufficient for a coordinate grid, I agree with Kato-san when it
comes to Milky Way fields or external galaxies. Since everyone seems to have the GSC or
USNO-A and a program like Astrometrica, it seems silly in the current age to not go ahead
and expand the scheme to the nearest arcsec. That, at least, handles almost all
ground-based cases.
Note that many programs (Hipparcos for example) have gone to a decimal degree format
in both coordinates. Since we are discussing a naming scheme that may be used for
many years in the future, perhaps we should consider such coordinates instead. In
addition, the ICRS is more-or-less J2000 Equinox, so we don't need to include an equinox
designator if ICRS is used.
I disagree with Taichi regarding a unique designator for variable stars. I would prefer
a single designation scheme for ALL objects, since there always cases where an object
is found to be variable after it is cataloged for some other purpose. Using a unique
scheme also removes the difficulty of a preliminary designation that later proves to
be false. The star remains; just its variability 'flag' is removed.
I confess we just used a running index for the FASTT variables because of that
scheme's convenience. I will make an effort to use an ra/dec scheme in the next paper!
Arne
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