homeostasis
发表于 2025-3-23 12:36:38
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needle
发表于 2025-3-23 14:36:12
Animal Models for Cardiac Valve Researchhe first type of interactions an expanding ring is formed, in a way similar to the formation of ring galaxies from a nonbarred target. Depending on the impact angle and position, the center of the bar may be temporarily offset from that of the disc..In the second type of interactions the companion i
镀金
发表于 2025-3-23 18:35:06
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争吵加
发表于 2025-3-24 01:04:56
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Paraplegia
发表于 2025-3-24 03:48:35
The Left Ventricle—General Considerations through gravitational instability to reach a hot quasi steady-state in the absence of gas. The latter is then the motor of evolution, and is at the origin of the formation of secondary structures, as rings, lenses or bars within bars. The evolution can be self-regulated, since too much gas concentr
Ovulation
发表于 2025-3-24 08:52:13
The Great Vessels and the Pericardiumity field across the whole nuclear and bar region. Strong unresolved (4″ or 700 pc) velocity discontinuities are observed across the dustlanes that we identify with large scale shocks observed in hydrodynamic simulations. Although hydrodynamical models are generally used to constrain the mass model,
乐章
发表于 2025-3-24 10:45:37
https://doi.org/10.1057/9780312299187sition. The observing grid has a 5″-spacing in the inner and a 10″-spacing in the outer region. A circumnuclear molecular torus with a radius of about 5″ is the dominant feature. Molecular emission is also seen coming from various dust streamers in the bar of the galaxy. The velocity field of the mo
epidermis
发表于 2025-3-24 17:27:12
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强行引入
发表于 2025-3-24 18:59:15
https://doi.org/10.1057/9780312299187o remarkable objects presented here, M 31 and M 104, display peculiar kinematics: a rapidly rotating cold nuclear disk and puzzling photometric and kinematical asymetries in the case of M 104 and M 31 respectively. Axisymmetric models confirm the presence of supermassive black holes. However at the
健谈的人
发表于 2025-3-25 01:39:31
https://doi.org/10.1057/9780312299187lationship to the active nucleus. We find that Seyferts are offset from the Faber-Jackson relation for normal galaxies having brighter bulges at a given velocity dispersion than normal galaxies. This indicates that Seyferts have lower mean mass-to-light ratios than normal galaxies and therefore youn