CCD Photometry of Faint Variable Stars in the Field of the Globular Cluster M4

Details CCD Photometry of Faint Variable Stars in the Field of the Globular Cluster M4 CCD Photometry of Faint Variable Stars in the Field of the Globular Cluster M4

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aj....113.2219k&link_type=abstract

Astronomical Journal v.113, p. 2219-2225 (1997)

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27

Scientific paper

We present the results of a photometric survey for faint variable stars in the nearby globular cluster M4. Twelve variables were discovered. Seven of the twelve are W Ursa Majoris stars that are probable members of the cluster. Another variable is faint blue degenerate star with 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 spectrum shows no emission lines.

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