Brh V128 is a Double-Mode High-Amplitude delta Scuti Star

Details Brh V128 is a Double-Mode High-Amplitude delta Scuti Star Brh V128 is a Double-Mode High-Amplitude delta Scuti Star

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ibvs.5552....1b&link_type=abstract

Information Bulletin on Variable Stars, 5552, 1.

Physics

1

Delta Scuti Stars, Double Mode Variability, Photometry

Scientific paper

CCD-V and unfiltered photometric data show that Brh V128 = GSC 1893-89
is a new high-amplitude double-mode Delta Scuti variable with a
fundamental period of 0.1534 days and a period ratio of 0.767. The
amplitude of the first overtone pulsation is slightly larger than that
of the fundamental mode.

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