J. Kaluzny et al., CCD PHOTOMETRY OF FAINT VARIABLE-STARS IN THE FIELD OF THE GLOBULAR-CLUSTER M4, The Astronomical journal, 113(6), 1997, pp. 2219-2225
We present the results of a photometric survey for faint variable star
s in the nearby globular cluster M4. Twelve variables were discovered.
Seven of the twelve are W Ursa Majoris stars that are probable member
s of the cluster. Another variable is a faint blue degenerate star wit
h a period of about 60 minutes, While the magnitude and colors of this
star are consistent with those of a cataclysmic variable in M4, a spe
ctrum shows no emission lines. (C) 1997 American Astronomical Society.