Dr. Klaus Bernhard - 13. Februar 2000
Bei meiner Veränderlichensuche konnte ich einen neuen vermutlichen
Algolstern entdecken:
GSC 736 1615; RA:6h 24m 54.0s DEC +10°14min 05sec (11.7-12.1 mag)
Um bestätigende Beobachtungen wird ersucht.
## BeV36
BeV36 062454.0 N101405 (J2000) 11.7 12.1(CCD)
comments:
BeV36: GSC 736 1615
Comparison star was for all measurements GSC 736 765 (11.9 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
GSC 736.1615 shows a single series of frequencies around 2.800
cycles/day and its one-day aliases.
This star is probably a weakly eclipsing variable
and the best period is probably 1.256 or 0.555 days (or twice
these).
object YYMMDD(UT) mag (CCD) code
BeV36 000111.9403 11.73 BRH.BAV
BeV36 000124.9174 12.10 BRH.BAV
BeV36 000125.9472 11.82 BRH.BAV
BeV36 000126.9444 11.72 BRH.BAV
BeV36 000127.9160 11.78 BRH.BAV
BeV36 000201.9076 11.74 BRH.BAV
BeV36 000203.9375 12.11 BRH.BAV
BeV36 000204.8840 11.72 BRH.BAV
BeV36 000210.9222 11.72 BRH.BAV