十二个数量级:从千秒差距到亚天文单位尺度探测星际介质
星系天体物理
2019-03-19 v1 天体物理仪器与方法
摘要
在理解气体流入、流出及穿过银河系方面取得十年重大进展后,我们正准备将观测与模拟相结合,以构建多尺度磁化星际介质(ISM)的综合图像。这些见解对于 2020 年代的四个大胆计划也至关重要:用脉冲星计时阵列(PTAs)探测纳赫兹引力波、破译快速射电暴(FRBs)、宇宙 B 模探测,以及用事件视界望远镜(EHT)对银河系黑洞成像。
引用
@article{arxiv.1903.07370,
title = {Twelve Decades: Probing the Interstellar Medium from kiloparsec to sub-AU scales},
author = {Dan Stinebring and Shami Chatterjee and Susan E. Clark and James M. Cordes and Timothy Dolch and Carl Heiles and Alex S. Hill and Megan Jones and Victoria Kaspi and Michael T. Lam and T. J. W. Lazio and Natalia Lewandowska and Dustin R. Madison and Maura A. McLaughlin and Naomi McClure-Griffiths and Nipuni Palliyaguru and Barney J. Rickett and Mayuresh P. Surnis},
journal= {arXiv preprint arXiv:1903.07370},
year = {2019}
}
备注
11 page, 6 figures, 47 references. Submitted as an Astro2020 science white paper on March 11, 2019