HATCH
发表于 2025-3-25 05:30:59
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xanthelasma
发表于 2025-3-25 09:06:23
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Coronary-Spasm
发表于 2025-3-25 13:29:57
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爱管闲事
发表于 2025-3-25 17:16:38
Judith Rauchociated MHD luminosity of ∽ — 10. — 10. erg s. . Bi-polar flows driven by this MHD power can affect or even cause the explosions associated with core-collapse supernovae. If the initial rotation is too slow, then there will not be enough rotational energy to power the supernova despite the high lumi
Meditative
发表于 2025-3-25 21:29:50
Sabine Deichsel-Steiningerer H . than the outer disks. Galaxies with lower luminosity (.14.5 mag) and star formation (SF) rate (SFR, log(SFR (.)) .2.1) tend to have steeper PS, which implies that the H . line-of-sight depths can be comparable with the radial length scales in low mass galaxies. A lack of a correlation between
1分开
发表于 2025-3-26 02:55:17
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使迷醉
发表于 2025-3-26 07:36:02
Johannes Wendlandlly) than those produced 30 years ago. This progress has been possible because of the introduction of large and fast electronic computers and the simultaneous development of an adequate numerical procedure connected with the name of L.G. Henyey. His method for calculating models in hydrostatic equil
dendrites
发表于 2025-3-26 08:55:28
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amputation
发表于 2025-3-26 12:42:56
Britta Binzerörtern durch . gewidmet, deren Genauigkeit allerdings hinter der von . erzielten erheblich zurückbleibt. Mit der weiteren Vervollkomnmung des zur Festlegung der Sternörter dienenden Meridiankreises und der Beobachtungs- und Reduktionsmethoden.) wuchs auch die Zahl der sich der Aufgabe der Bestimmung
Cardioversion
发表于 2025-3-26 17:42:08
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