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Relationship between Environment and the Broadband Optical Properties of Galaxies in the Sloan Digital Sky Survey*

机译:斯隆数字天空调查中环境与星系宽带光学特性之间的关系*

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摘要

We examine the relationship between environment and the luminosities, surface brightnesses, colors, and profile shapes of luminous galaxies in the Sloan Digital Sky Survey (SDSS). For the SDSS sample, galaxy color is the galaxy property most predictive of the local environment. Galaxy color and luminosity—measures of the star formation history—jointly comprise the most predictive pair of properties. At fixed luminosity and color, density is not closely related to surface brightness or to Sérsic index—measures of galaxy structure. In the text, we discuss what measurable residual relationships exist, generally finding that at red colors and fixed luminosity, the mean density decreases at the highest surface brightnesses and Sérsic indices. In general, these results suggest that the structural properties of galaxies are less closely related to galaxy environment than are their masses and star formation histories.
机译:我们在斯隆数字天空调查(SDSS)中检查了环境与发光星系的亮度,表面亮度,颜色和轮廓形状之间的关系。对于SDSS样本,星系颜色是最能预测本地环境的星系属性。星系的颜色和光度-恒星形成历史的量度-共同构成了最具预测性的一对属性。在固定的亮度和颜色下,密度与表面亮度或Sér​​sic指数(银河结构的度量)没有密切关系。在本文中,我们讨论了存在哪些可测量的残留关系,通常会发现在红色和固定亮度下,平均密度在最高表面亮度和Sérsic指数下会降低。通常,这些结果表明,与质量和恒星形成历史相比,星系的结构特性与星系环境之间的关系不那么紧密。

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