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[vsnet-newvar 1705] GSC 05154-01249 is a Mira variable
- Date: Wed, 4 Dec 2002 15:37:29 -0800 (PST)
- To: vsnet-newvar <vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp>, Stardial <pmcc@astro.uiuc.edu>
- From: Patrick Wils <patrickwils@yahoo.com>
- Subject: [vsnet-newvar 1705] GSC 05154-01249 is a Mira variable
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
Stardial (http://vsnet.astro.uiuc.edu/stardial/) images between 1999 and
2002, show that GSC 05154-01249 is a Mira variable with a period of 290
days. Only data near maximum is recorded on the images.
The NOFS plate archive was checked
(http://vsnet.nofs.navy.mil/data/fchpix), showing a B-R value of about
+3, and a difference of 2 magnitudes between the two red plates,
confirming variability. There is a close companion about 5" West.
Other identifications (using the VizieR utility at the CDS in
Strasbourg, http://vizier.u-strasbg.fr/cgi-bin/VizieR) :
IRAS 19456-0522
IRASF 19457-0522
USNO-A2.0 0825-17001301
USNO-B1.0 0847-0554572
GSC2.2 S3021302193
2MASS entry : J = 6.521, H = 5.543, K = 4.893
Coordinates: 19 48 21.3500 -05 15 06.790 (USNO-B1.0)
To reduce the Stardial images, use was made of programs written by
Michael Richmond (see http://vsnet.tass-survey.org).
Patrick
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