万灵药
发表于 2025-3-21 17:07:09
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用手捏
发表于 2025-3-21 20:55:15
Advances in Science, Technology & Innovationot show a tendency for the amplitudes to grow. Perhaps including time-dependent convection and/or modeling deeper envelopes with additional radiative damping will limit the pulsation amplitudes to observed values.
终点
发表于 2025-3-22 00:42:51
Advances in Science, Technology & Innovationch may have a sequential evolutionary connection. For the Wolf Rayet stars the Luminous Magnetic Rotator model may be able to explain the long standing “wind momentum problem” as well as the “spin-down problem” associated with earlier rotating wind models. Constraints on the surface magnetic field a
Factorable
发表于 2025-3-22 07:07:23
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外来
发表于 2025-3-22 09:38:07
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装饰
发表于 2025-3-22 13:34:34
Pulsation Studies of a 1.8 M⊙ Delta Scuti Modelot show a tendency for the amplitudes to grow. Perhaps including time-dependent convection and/or modeling deeper envelopes with additional radiative damping will limit the pulsation amplitudes to observed values.
造反,叛乱
发表于 2025-3-22 20:55:03
Basic Magnetic Rotator Theory with Application to the Angular Momentum Driven Winds of B and Wolfch may have a sequential evolutionary connection. For the Wolf Rayet stars the Luminous Magnetic Rotator model may be able to explain the long standing “wind momentum problem” as well as the “spin-down problem” associated with earlier rotating wind models. Constraints on the surface magnetic field a
轻浮女
发表于 2025-3-23 01:04:55
Constraints on the Thickness of be Star Disks Derived from Combined IR Excess and Optical Polarimetron envelope, or by having partial cancellation of the equatorial polarization from contributions near the pole. The two solutions have different base densities, .., and may be differentiated by yet other observational data.
growth-factor
发表于 2025-3-23 05:00:33
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Conducive
发表于 2025-3-23 09:20:37
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