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Seismology of the Sun and the Distant Stars - Using Today's Successes to Prepare the Future – TASC2 & KASC9 Workshop – SPACEINN & HELAS8 Conference, Date: 2016/07/10 - 2016/07/15, Location: Azores

Publication date: 2017-10-27
Volume: 160
Publisher: EPJ Web of Conferences

Seismology of the Sun and the Distant Stars - Using Today's Successes to Prepare the Future – TASC2 & KASC9 Workshop – SPACEINN & HELAS8 Conference

Author:

Bowman, Dominic M
Kurtz, Donald W ; Breger, Michel ; Murphy, Simon J ; Holdsworth, Daniel L ; Monteiro, MJPFG ; Cunha, MS

Keywords:

Science & Technology, Physical Sciences, Astronomy & Astrophysics, SCUTI, 5107 Particle and high energy physics, 5110 Synchrotrons and accelerators

Abstract:

The results of a search for amplitude modulation of pulsation modes in 983 δ Sct stars, which have effective temperatures between 6400 ⩽ Teff ⩽ 10 000 K in the Kepler Input Catalogue and were continuously observed by the Kepler Space Telescope for 4 yr, are presented. A total of 603 δ Sct stars (61.3 per cent) are found to exhibit at least one pulsation mode that varies significantly in amplitude over 4 yr. Furthermore, it is found that amplitude modulation is not restricted to a specific region within the classical instability strip in the HR diagram, therefore its cause is not necessarily dependent on stellar parameters such as Teff or log g. On the other hand, many δ Sct stars show constant pulsation amplitudes demonstrating that the cause of pulsational non-linearity in these stars is not well understood.