乐意
发表于 2025-3-26 21:50:18
Wolf-Michael Kählert reach to the evolutionary state of the nebula where planet formation is expected. Interestingly the most far reaching calculations point to nebulae, that are initially below the so called minimum reconstituted mass (Morfill et al. 1985).
受伤
发表于 2025-3-27 02:26:17
Wolf-Michael Kählere so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been978-94-007-3242-1978-90-481-8687-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
decode
发表于 2025-3-27 05:25:53
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Compassionate
发表于 2025-3-27 11:04:27
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公式
发表于 2025-3-27 14:25:02
e so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been978-94-007-3242-1978-90-481-8687-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
GUILT
发表于 2025-3-27 18:04:24
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不给啤
发表于 2025-3-27 23:48:09
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比目鱼
发表于 2025-3-28 03:37:20
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ARM
发表于 2025-3-28 07:22:03
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食道
发表于 2025-3-28 12:11:47
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