假
发表于 2025-3-28 17:25:26
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/b/image/186289.jpg
从容
发表于 2025-3-28 22:26:43
Disk Instabilities in Hubble-Sandage Variables? Observations by Tamman and Sandage (1968) and Rosino and Bianchini (1973) followed. The main characteristics are high luminosity (L/L⊙ ≈ 10.), blue color indices, F type spectra and irregular variability.
跑过
发表于 2025-3-28 23:01:19
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我怕被刺穿
发表于 2025-3-29 05:20:57
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注视
发表于 2025-3-29 10:33:59
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似少年
发表于 2025-3-29 13:49:07
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受辱
发表于 2025-3-29 18:34:04
Evolution of Stars in the Post-Main Sequence Stageossible to fit a convective core into the point source model of stellar structure integrated by Cowling three years earlier. The free parameter in the fitting process could be fixed with the thermonuclear reaction rates, the first realistic stellar model for a massive main sequence star was construc
疼死我了
发表于 2025-3-29 20:17:11
Disk Instabilities in Hubble-Sandage Variables? Observations by Tamman and Sandage (1968) and Rosino and Bianchini (1973) followed. The main characteristics are high luminosity (L/L⊙ ≈ 10.), blue color indices, F type spectra and irregular variability.
abduction
发表于 2025-3-30 00:50:49
The Frequency of Cepheid Binariesent photometric method proposed by Fernie (1980). If applied to the set of VBLUW observations of southern Cepheids carried out by Pel (1976), this method gives a frequency of about 25%, which is consistent with the more recent spectroscopic determinations (Gieren, 1981). The importance of the IUE sa
sed-rate
发表于 2025-3-30 06:44:17
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