[vsnet-recent-rr 858] Re: V1032 Oph

[Wolfgang Renz]

Hello

FYI again.

V1032 Oph is NOT an uncertain RR Lyr star !!!
Its an UGSU+E star with eclipses of ~ 0.5 to 0.8 mag.

Could you please change the outdated GCVS var type classification
of V1032 Oph (that originats from 1965) from "RRAB:" to "UGSU+E"
and drop it from the internal RR Lyr lists ?
Thx.

outdated GCVS entry:
http://www.sai.msu.su/gcvs/cgi-bin/search.cgi?search=V1032+Oph

VSX entry:
http://www.aavso.org/vsx/index.php?view=detail.top&oid=21518

outburst notification of March, 2010:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11898
eclipse detection announcement:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11904
original eclipse detection and first period guess:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11905
further data by discoverer and improved period:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11907
first elements with improved period, first superhump period:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11909
improved elements:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11912
improved superhump period:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11918
improved superhump period:
http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/11931

Clear skies
 Wolfgang

-- 
Wolfgang Renz, Karlsruhe, Germany