Fw: [AAVSO-DIS] T Leo renaming

Julian Parks Feb 27, 2007

Greetings Group. Several members on the AAVSO discussion site have been
wrangling also with the issue of variable star nomenclature as well as Guide
users. See the AAVSO Director, Arne Henden's, e-mail below.

Julian Parks

----- Original Message -----
From: "arne" <arne@...>
To: "Robert J. Modic" <rjmodic@...>
Cc: "AAVSO-Discussion" <aavso-discussion@...>
Sent: Tuesday, February 27, 2007 1:07 PM
Subject: Re: [AAVSO-DIS] T Leo renaming


> Robert J. Modic wrote:
>> Last year, a number of variables that are located close
>> to constellation boundaries were renamed. These variables
>> were discovered before the adoption of modern constellation
>> boundaries and they wound up being located in adjacent
>> constellations. The problem is that many of these stars,
>> T Leo being a prime example, have been observed for a long
>> time with many papers published using the original
>> designations. The history of variable star nomenclature is
>> complicated enough without confusing the issue further. I
>> have heard very little discussion about this renaming.
>> What was the justification for this decision? What is the
>> AAVSO's position on this? Is there a way to appeal this?
>>
> Nicolai Samus (head of GCVS) announced the name changes in
> Astronomy Letters (2006, vol32n4, pp263-273): "Electronic
> Version of the Third Volume of the General Catalogue of
> Variable Stars with Improved Coordinates." The GCVS team
> spent a number of years, pouring over the 3rd edition, looking
> up photos and identifications (including asking Martha Hazen
> for a lot of the Harvard Variables, which is why she and
> David Williams, our President, are coauthors of this paper).
> They also relied on other sources, such as ASAS, to ensure
> the correct variable with proper type and period was identified.
> They were largely successful, and this was an enormous effort,
> with about 40,000 stars being examined.
>
> Once they had the variables properly identified, they used UCAC
> and 2MASS to get accurate coordinates. For a couple of hundred
> stars, they were unable to find the star, and they can be
> considered "lost".
>
> This paper is fun to read, especially the "Comments on some of
> the problem stars of the electronic version."
>
> However, what is relevant to this topic is that they included
> Table 3, a list of GCVS stars in wrong constellations. About
> 38 stars were incorrectly assigned to a constellation; most
> because the submitted coordinates were so poor that the GCVS
> staff made the wrong assignment. Some are more than 10 degrees
> from their proper position (lots of fun identifying those variables,
> I bet!). T Leo is one of those stars with poor coordinates.
> In fact, it is the most widely known of the list since most of the
> rest were so badly positioned that no one observed them.
>
> In 1930, the IAU took the opposite approach: they changed the
> constellation
> boundaries so that 6 variables remained within the constellations they
> were
> originally named for! It would be very hard to do that today.
>
> Samus' position is that, if he was going to correct 37 other stars,
> he didn't want to make an exception for T Leo. The 78th Name-List
> of Variable Stars (IBVS 5721, 8 August 2006) repeated this list
> as its Table 2. In addition, Samus' powerpoint presentation makes
> the point that, while the stars have been given new names, their
> old names have been removed from circulation and will not be
> reassigned. This means you are not prevented from using the old
> name, just that the new name is preferred for all new publications.
>
> My position, presented to Samus in email and at the IAU meeting,
> is that a name is just that - a name. Constellations are large,
> and there will always be a few cases of misidentification. I'd rather
> leave the names as-is rather than assigning a new name and creating
> a new paper trail. Samus was unswayed, and since his group gets
> to assign names, he wins. However, a new working group of the IAU
> has been started to look into naming conventions and especially to
> resolve the proliferation of classification names, so perhaps some
> resolution of the issues will take place before the next IAU meeting
> in 2009.
> Arne
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