高红移宇宙中尘埃渗透形态
天体物理学
2016-01-27 v2
摘要
来自哈勃深场(HDF)北和南的图像显示出大比例的尘埃覆盖的高红移星系，其外观超出传统分类系统。这些对象的本质尚未完全理解。由于HDF优先抽样restframe UV光，HDF形态并非尘埃或'mask'渗透。高红移星系在近红外restframe下的外观仍是 New Millennium 的挑战。下一代太空望远镜(NGST)可能常规提供此类图像。在本稿件中，我们定量确定了高红移星系（如NGC 922）在其近红外restframe中的尘埃渗透结构。我们展示，此类光学异常星体可使用Block和Puerari(1999)以及Buta和Block(2001)的尘埃渗透 z ~ 0 模板进行分类。
引用
@article{arxiv.astro-ph/0106483,
title = {Dust penetrated morphology in the high redshift Universe},
author = {D. L. Block and I. Puerari and M. Takamiya and R. Abraham and A. Stockton and I. Robson and W. Holland},
journal= {arXiv preprint arXiv:astro-ph/0106483},
year = {2016}
}
备注
4 pages, 2 figures. Presented at the conference "The Link between Stars and Cosmology", 26-30 March, 2001, Puerto Vallarta, Mexico. To be published by Kluwer, eds. M. Chavez, A. Bressan, A. Buzzoni, and D. Mayya. High-resolution version of Figure 2 can be found at http://www.inaoep.mx/~puerari/conf_puertovallarta