Jun 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..383k&link_type=abstract
Communications in Astroseismology, Vol. 150, p.383
Other
1
Scientific paper
A large CCD photometry observing campaign in search of p mode
oscillations in K giants (see Frandsen et al. 2007) has produced very
high quality time series data for the RR Lyrae stars and other variables
in the globular cluster M4. New variables have been found and the known
RR Lyrae stars have been better characterized.
Frandsen Soeren
Kopacki Grzegorz
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