recession 发表于 2025-3-28 18:11:50
Characterising Pulsational Non-linearity,odels providing no predictive power of pulsation mode amplitudes. In this chapter, the non-linearity of pulsations in . Sct and gamma Dor stars is investigated, which includes the application of mode coupling models to determine the strength of non-linearity in a selection of pulsating stars. FurtheStatins 发表于 2025-3-28 18:50:45
Investigating the HADS Stars with , Data,3 mag and predominantly pulsate in the fundamental and/or first overtone radial p modes. These stars are rare, making up less than one per cent of pulsating stars in the classical instability strip. In this chapter, the only two HADS stars observed by the . Space Telescope are studied, including detGeneric-Drug 发表于 2025-3-29 00:45:11
http://reply.papertrans.cn/16/1548/154756/154756_43.pngRAFF 发表于 2025-3-29 05:11:27
http://reply.papertrans.cn/16/1548/154756/154756_44.png