超大质量黑洞的宇宙演化：未来二十年的展望
星系天体物理
2019-03-28 v1
摘要
过去 20 年间，Chandra 与 XMM-Newton 巡天结合同天区的多波段成像与光谱数据所做出的发现，显著改变了关于超大质量黑洞（SMBH）与星系关联的认识。这些发现提出了若干超出当前 X 射线望远镜能力范围的激动人心的问题，需在今后二十年的天文台予以解决。随着新天文台窥探早期宇宙，我们将开始理解 SMBH 婴儿期（在 ）的物理性质与人口统计，并探究其吸积对首批星系形成的影响（ 2.1）。我们还将能理解星系中全部黑洞种群在宇宙历史（在 1-6）中的吸积与演化，包括低吸积率、重度遮蔽的 AGN，其光度超出当前 X 射线巡天所能触及的范围（2.2 与 2.3），从而使我们能够解析 SMBH 增长与其环境之间的联系。
引用
@article{arxiv.1903.11091,
title = {Cosmic evolution of supermassive black holes: A view into the next two decades},
author = {Francesca Civano and Nico Cappelluti and Ryan Hickox and Rebecca Canning and James Aird and Marco Ajello and Steve Allen and Eduardo Bañados and Laura Blecha and William N. Brandt and Marcella Brusa and Francisco Carrera and Massimo Cappi and Andrea Comastri and Klaus Dolag and Megan Donahue and Martin Elvis and Giuseppina Fabbiano and Francesca Fornasini and Poshak Gandhi and Antonis Georgakakis and Kelly Holley-Bockelmann and Anton Koekemoer and Andrew Goulding and Mackenzie Jones and Sibasish Laha and Stephanie LaMassa and Giorgio Lanzuisi and Lauranne Lanz and Adam Mantz and Stefano Marchesi and Mar Mezcua and Beatriz Mingo and Kirpal Nandra and Daniel Stern and Doug Swartz and Grant Tremblay and Panayiotis Tzanavaris and Alexey Vikhlinin and Fabio Vito and Belinda Wilkes},
journal= {arXiv preprint arXiv:1903.11091},
year = {2019}
}
备注
5 pages, 3 figures; Science white paper submitted to the Astro2020 Decadal Survey