白矮星周围的行星系统

D. Veras
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引用次数: 10

摘要

白矮星行星科学是一个快速发展的研究领域,以各种观测和理论探索为特色。巨行星、小行星和碎片盘都被发现围绕白矮星运行。破碎的小行星的内部以元素为基础进行测量,提供了一种独特的系外行星化学探测。数值模拟和分析研究追踪了这些系统的剧烈物理和动力学历史,从天文单位(au)尺度的距离到白矮星的直接邻近,在那里,小行星被分解成尘埃和气体,并吸积到白矮星光球上。目前和即将到来的地基和天基仪器可能会进一步加快发现的步伐。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Planetary Systems Around White Dwarfs
White dwarf planetary science is a rapidly growing field of research featuring a diverse set of observations and theoretical explorations. Giant planets, minor planets, and debris discs have all been detected orbiting white dwarfs. The innards of broken-up minor planets are measured on an element-by-element basis, providing a unique probe of exoplanetary chemistry. Numerical simulations and analytical investigations trace the violent physical and dynamical history of these systems from astronomical unit (au)-scale distances to the immediate vicinity of the white dwarf, where minor planets are broken down into dust and gas and accrete onto the white dwarf photosphere. Current and upcoming ground-based and space-based instruments are likely to further accelerate the pace of discoveries.
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