银河系高海拔的尘埃破坏

E. Sivkova, D. Wiebe
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引用次数: 0

摘要

由于不同大小的尘埃粒子的相对运动,考虑了被辐射压力扫向近星系空间的碳质尘埃粒子被破坏的可能性。在辐射压力、重力和气体阻力的作用下,星系中尘埃运动的早期模型被扩展到考虑到破坏过程。考虑到它与银河系气体和其他尘埃粒子的碰撞,人们考虑了清扫尘埃的可能性。此外,我们还澄清了由于所描述的机制而可以进入星系间空间的粒子大小的范围。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dust destruction at high galactic altitude
The possibility of destruction carbonaceous dust particles swept out by the radiation pressure into near-galactic space due to the relative motion of dust particles of various sizes is considered. The earlier model of the motion of dust in the Galaxy under the action of radiation pressure, gravity, and gas resistance is expanded taking into account the destruction processes. The possibility of dust sweeping is considered taking into account its collisions with the gas of the Galaxy and with other dust particles. Also, we clarify the range of particle sizes that can get into intergalactic space due to the described mechanism.
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