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Showing 1 to 2 of 2 for “"instability strip"”.
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Investigating the A-type stars using Kepler data
… 56 per cent. The non-δ Sct stars in the δ Sct instability strip receive far less attention. Some of these stars, without appreciable granulation or stellar winds, are probably the least variable objects on the HR diagram. It is shown that they have the potential to be among the most peculiar Am …
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A Search for Low-Amplitude Variability Among Population I Main Sequence Stars
The detection of variable stars in open clusters is an essential component of testing stellar structure and evolution theories. The ability to detect low-amplitude variability among cluster members is directly related to the quality of the photometric results. Point Spread Function (PSF) fitting is …