corpus-callosum
发表于 2025-3-25 06:56:03
and is poorly approximated as a power law. Current results in this area are at best provisional. Despite these uncertainties, however, and even given the current low-accuracy abundance estimates, we can use late-type subdwarfs as calibrators in main sequence fitting. The initial results from that a
Largess
发表于 2025-3-25 09:39:45
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POWER
发表于 2025-3-25 13:14:28
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违法事实
发表于 2025-3-25 17:47:40
Constantinos Frangos PhD are that gas giants form more readily at super-solar metallicities, although ∼5% of sun-like stars have detectable companions. Lower mass stars also have planetary companions, as emphasised by the discovery of planets around Gl 876 and Gl 836, although the overall frequency of Jovian-mass gas giant
Invigorate
发表于 2025-3-25 22:48:52
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Traumatic-Grief
发表于 2025-3-26 00:22:02
Constantinos Frangos PhD are that gas giants form more readily at super-solar metallicities, although ∼5% of sun-like stars have detectable companions. Lower mass stars also have planetary companions, as emphasised by the discovery of planets around Gl 876 and Gl 836, although the overall frequency of Jovian-mass gas giant
马具
发表于 2025-3-26 04:26:56
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HALO
发表于 2025-3-26 11:44:08
Constantinos Frangos PhDtle should be interpreted accordingly. The expression ‘low-mass stars‘ carries a wide range of meanings in the astronomical literature, but is most frequently taken to refer to objects with masses comparable with that of the Sun - F and G dwarfs, and their red giant descendants. While this definitio
PAN
发表于 2025-3-26 12:48:53
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ARM
发表于 2025-3-26 17:26:35
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