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Science in crowded fields with Hubble Space Telescope Faint Object Spectrograph plus COSTAR

机译:拥挤领域的科学与哈勃太空望远镜微弱的物体光谱仪加上肋骨

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We describe plans for several science programs in crowded fields using the faint object spectrograph (FOS) which rely critically on the enhanced angular resolution provided by the COSTAR corrective optics. Based on ground-based calibration of the COSTAR and on-orbit performance of the FOS, the anticipated performance of the COSTAR$PLU/FOS should allow many important scientific studies to be completed which have had to be postponed due to the spherical aberration in the HST primary mirror. Particularly impacted by spherical aberration, and thus able to benefit most dramatically from the installation of COSTAR, are spectroscopic observations with FOS in crowded fields. Many of the most important science goals for the FOS instrument involve observations of crowded fields, for which the restored high- angular resolution of HST is essential - not only to isolate features of small angular extent, but also to eliminate optical contamination from the surrounding luminous regions. Spectroscopy of the nuclei of galaxies to obtain rotation curves and velocity dispersions which might reveal the presence of central black holes benefits dramatically from the enhanced angular resolution of HST as restored by COSTAR. We present models based on our current understanding of the dynamics of galaxy nuclei to illustrate the dramatic improvement in sensitivity in searching for black holes made possible by restoring HST's image quality. Two other categories of scientific investigations in crowded fields which will benefit greatly from restoring HST's image quality are spectroscopy of the luminous material (presumably distant galaxies) surrounding quasistellar objects, and spectroscopy of individual stars in globular clusters. The promise of finally being able to carry out these exciting scientific programs with the FOS on the restored HST explains why our team of scientists, along with many other astronomers, look forward to using the restored HST to carry out the scientific investigations for which it was originally intended.
机译:我们使用微弱的物体光谱仪(FOS)描述拥挤领域在拥挤的领域的几个科学计划的计划,其依赖于Costar纠正光学系统提供的增强的角度分辨率。基于FOS的地面校准和FOS的轨道表现,肋骨$ PLU / FOS的预期表现应允许许多重要的科学研究才能完成,这些研究必须由于球形差距而被推迟HST主镜子。特别受到球面像差的影响,从而能够从肋骨的安装中急剧受益,是具有拥挤领域的FOS的光谱观察。 FOS仪器的许多最重要的科学目标涉及对拥挤领域的观察,其中HST的恢复高角度分辨率是必不可少的 - 不仅要隔离角度小的特征,还可以消除来自周围发光的光学污染地区。星系的核的光谱学,获得旋转曲线和速度分散体,其可能揭示中央黑洞的存在,从Costar恢复的HST的增强的角度分辨率显着地显着。我们基于我们目前对Galaxy核的动态的理解,提出了通过恢复HST的图像质量来搜索可能的敏感性敏感性的显着改善。在拥挤的领域中,将从恢复HST的图像质量受益的其他两类科学调查是围绕Quasistellar对象的发光材料(概要星系)的光谱,以及球状簇中的个体恒星的光谱。最终能够在恢复的HST上与FOS执行这些令人兴奋的科学计划的承诺解释了为什么我们的科学家团队以及许多其他天文学家一起期待使用恢复的HST来执行它的科学调查最初的意图。

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