New variable stars in the globular cluster M4

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Globular Clusters, Red Giant Stars, Variable Stars, Color-Magnitude Diagram, Stellar Spectrophotometry

Scientific paper

The DAOPHOT program was used to study the globular cluster M4 in order to confirm previous observations of variability made by photographic methods. A variable star with periodicity in the middle part of the red giant branch (RGB) was observed. Three other variables may be members of a new subgroup of RR Lyrae stars in globular clusters. Another star is found to be located at the intersection of the RGB and the horizontal branch.

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