On the period variability of GP andromedae |
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Authors: | Alexandru Pop Victor Liteanu Dan Moldovan |
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Institution: | (1) Astronomical Observatory Cluj-Napoca, Astronomical Institute of the Romanian Academy, Str. Cireşilor 19, RO-3400 Cluj-Napoca, Romania;(2) Faculty of Chemistry and Chemical Engineering, Babeş-Bolyai University, Str. Arany Janos 11, RO-3400 Cluj-Napoca, Romania |
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Abstract: | The present paper deals with the pulsation period variability of the high-amplitude δ Scuti star GP Andromedae using a data
set covering a time base of 26.9 years. The possibility of a periodic component (reflecting the light-time effect induced
by a hypothetic binarity) in the O-C curve is inferred. The presence of this periodicity in the period variation of GP And leads to a diminution of the discrepancy
between predicted and observed relative period change rates. The hypothesis of the existence of an unseen companion is discussed.
The statistical analysis of the final O-C residuals distribution, indicates their normal or close to normal character.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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