我要威胁
发表于 2025-3-30 09:48:52
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critic
发表于 2025-3-30 13:39:11
The Spectroscopic Observations of CoRoT Asteroseismic Targets with HARPSPS spectrograph attached to the 3.6m-ESO telescope in the framework of two consecutive Large Programmes. We discuss its use to study line-profile variations and we report on a specific result obtained for the δ Sct star HD 170699.
hauteur
发表于 2025-3-30 17:24:49
Recent Progress and Open Questions in Rapidly Rotating Star Seismologyta together with the advances in modelling the effects of rotation bring fresh perspectives towards a successful comparison between theory and observation. In this short review, the recent progress obtained with 2D oscillation codes is summarized and some open issues are pointed out.
creatine-kinase
发表于 2025-3-30 23:54:26
Traditional Approximation for Low-Frequency Modes in Rotating Stars and A Working Hypothesis About Ece of eigenfunction is expressed in terms of the Hough functions, and the radial dependence is expressed in a form similar to the case of non-rotating stars with only the replacement of the spherical degree with the eigenvalue of the Hough function. Paying attention to the non-zero surface temperatu
刺穿
发表于 2025-3-31 01:12:19
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Ambiguous
发表于 2025-3-31 07:16:20
Regular Modes in Rapidly Rotating Stars asymptotic method for pressure modes predicts regular frequency spacings in the spectrum of rapidly rotating stars. We give a semi-analytical formula for these spacings that is in good agreement with numerically computed high-frequency modes. This should help to extract from observed spectra import