APS -APS March Meeting 2017 - Event - Explaining the Observed Relationships between the Dark Matter Halo Parameters and Half-Light Radii of Galaxies.

Benjamin Woodall; Casey Watson; Hunter Somers; Zech Miller

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APS -APS March Meeting 2017 - Event - Explaining the Observed Relationships between the Dark Matter Halo Parameters and Half-Light Radii of Galaxies.

机译：APS -APS 2017年3月会议-活动-解释暗物质晕参数与星系半光半径之间的可观测关系。

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We consider the relationships between the half-light radii and best-fit, Burkert dark matter halo parameters, which hold for Milky Way dwarf spheroidal galaxies (dSphs) as well as dwarf disks, spirals, and ellipticals over many orders of magnitude in galaxy size, mass, and luminosity. We report on possible mechanisms that could link the luminous and dark matter distributions of such a wide range of galaxy masses and types, and lie at the heart of these relationships.~

机译：我们考虑半光半径和最适合的伯克特暗物质光晕参数之间的关系，该参数适用于银河系矮球形球星系（dSphs）以及矮星盘，旋涡和椭圆星系，其大小超过了银河系大小的多个数量级，质量和亮度。我们报告了可能的机制，这些机制可以将如此广泛的星系质量和类型的发光和暗物质分布联系起来，并且位于这些关系的核心。

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《Bulletin of the American Physical Society》 |2017年第4期|共页
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Benjamin Woodall; Casey Watson; Hunter Somers; Zech Miller;
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1. APS -APS March Meeting 2017 - Event - The Observed Scaling Relationships between the Dark Matter Halo Parameters and Half-Light Radii of Multiple Galaxy Types. [J] . Zechariah Miller, Hunter Somers, Ben Woodall, Bulletin of the American Physical Society . 2017,第4期

机译：APS -APS 2017年3月会议-事件-多种银河系类型的暗物质光晕参数和半光半径之间的可观测比例关系。
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APS -APS March Meeting 2017 - Event - Explaining the Observed Relationships between the Dark Matter Halo Parameters and Half-Light Radii of Galaxies.

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