Measuring the period of the delta Scuti variable U1425-01208594 in Cassiopeia
Jeremy Shears, David Boyd, Steve Brady, Ian Miller, Roger Pickard
TL;DR
This paper reports the measurement of the pulsation period of the delta Scuti star U1425-01208594 in Cassiopeia, providing precise photometric data to characterize its variability.
Contribution
The study provides the first detailed measurement of the star's pulsation period and amplitude, confirming its classification as a delta Scuti variable.
Findings
Measured period of 0.06695 days
Amplitude of 0.014 mag
Supports delta Scuti classification
Abstract
The variability of U1425-01208594 was recently discovered by Schmidtobreick et al, who suggested that it is a member of the delta Scuti family of pulsating stars. Photometry conducted by the authors revealed a period of 0.06695(8) d and a peak-to-peak amplitude of 0.014 mag.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Geomagnetism and Paleomagnetism Studies