fibula
发表于 2025-3-27 00:43:29
Ph. Stee,D. Bonneau,D. Mourard,F. Vakiliestört, mögen auch die einzelnen mechanischen Fördereinrichtungen für sich durchaus einwandfrei arbeiten. Es kann daher nicht genug auf die wichtige Bedingung hingewiesen werden, daß die Neigung der Ladeschurren und schrägen Behälterböden sorgfältig dem Fördergut angepaßt werden muß. Dabei ist zwisc
Disk199
发表于 2025-3-27 01:51:39
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四指套
发表于 2025-3-27 06:06:17
Using spectropolarimetry to determine envelope geometry and test variability models for hot star ciFurthermore, spectropolarimetric variability, which is significant in a large fraction of the hot stars observed, provides information about changes occuring in the circumstellar envelope. For example, polarimetric changes provide a critical test of the one-armed density wave models proposed to explain observed V/R variations.
ANTH
发表于 2025-3-27 12:53:24
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ARBOR
发表于 2025-3-27 16:58:48
Rotationally modulated winds of O stars,hree case studies are used to illustrate the patterns of variability that are attributed to rotational modulation and to highlight some open issues connected with this hypothesis. The problems associated with establishing the occurrence of rotational modulation rigorously are also discussed.
DEFER
发表于 2025-3-27 19:17:04
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佛刊
发表于 2025-3-28 00:57:55
Non-isotropic outflows in the infrared: ISO imaging of LBVs,ed. The structure and intensity distribution of the nebular emission is dependent on the wavelength, indicating a separation between the ionised matter and the dust in the nebulae. Some model calculations are presented for the G79.29+0.46 nebula.
heterodox
发表于 2025-3-28 02:46:49
0075-8450 ere is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evoluti
盘旋
发表于 2025-3-28 06:46:00
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BOLT
发表于 2025-3-28 10:46:03
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