Release 11.12 ("Hergest Ridge")
NOTE: these info are added by user of the GGC-DB |
Number of comments available so far: 1
With the idea to search, measure and to determine the
present parameters of new variable stars in M13 we
have studied M13 during a period of 521days (of DJ
2.452.076 to DJ 2.452.596, both inclusively), and
measured during 129 nights (DJ 2.452.076 to 52.204) in
2001, and other 189 nights (DJ 2.452.408 to 52.596) in
2002 the brightness of 35 different stars between
variable, suspected variable and comparison stars,
with telescopes of 30.2 and 20.3-cm, and CCD cameras
(filter V Johnson), from Spain.
We have light curves of brightness, periodogram and
measurements of L629 that characterize it as a new
variable star of Red Giante type.
Date: 2003-02-18
From: Francisco Violat BordonauCluster: NGC 6205
Subject: Variability of L629 confirmed
We have confirmed the variability of L629, a new
variable star Red Giant (suspected variable star from
2000, June, in Osborn's paper), located in M13.
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