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[vsnet-chat 1336] Re: Designation of new variable stars
- Date: Sun, 27 Sep 1998 11:54:32 +0900 (JST)
- To: samus@sai.msu.su, vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 1336] Re: Designation of new variable stars
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: [vsnet-chat 1335] Re: Designation of new variable stars
Brian Skiff wrote:
> It would seem to me that if there is no designation from an ordinary
> catalogue (I would include the GSC and A1.0 as among these), the most
> convneient temporary designations are those based on coordinates, something
> like: J123456+1234.5, where the position is given to the precision of
> one time-second in RA and 0'.1 in Dec. This enough "resolution" to prevent
> problems nearly always, and avoids ad hoc designations such as "Peg2" that
> clutter the literature. It is preferable to include a designator as a
> prefix as well, so the recent discoveries could be something like:
> "BAO J232845+2834.1" or "KAIT ...." (just making up the numbers).
My chief concern is why there is no official tentative designating
policy for newly discovered variable stars. J123456+1234.5 may be acceptable
(and I indeed use this kind of new designations), but is not apparent it
points to a variable star. There may be number of nearby stars which are
within the same designation grid, esp. in the Milky Way field.
The name "BAO J232845+2834.1" may have the similar disadvantage: there is
no assureance the BAO team will use this designation strategy other than
variable stars. This may lead to an acronym collision from the same source
of information. I presume the best resolution is the GCVS team assign a
new variable star-specific acronym, and provide a naming strategy, and
encourage the CBAT or IBVS, in which reports most likely appear, to use
this naming policy. Otherwise (even if we constrain ourselves to use
J-numbered designations) there will be a number of observations of
"new cataclysmic variable in Peg" by other consortia.
Regards,
Taichi Kato
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