Measuring supermassive black holes via reverberation mapping in the UV

被引：1

作者：

Kaspi, Shai ^{[1
,2
]}

机构：

[1] Tel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Sch Phys & Astron, IL-69978 Tel Aviv, Israel

[2] Tel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Wise Observ, IL-69978 Tel Aviv, Israel

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2018年 / 363卷 / 04期

关键词：

Quasars; Black holes; Reverberation mapping; Broad line region; AGN; ACTIVE GALACTIC NUCLEI; BROAD-LINE REGION; SEYFERT-GALAXIES; CENTRAL MASSES; SIZE; STEPS; VARIABILITY; LUMINOSITY; CONTINUUM; QUASARS;

D O I：

10.1007/s10509-018-3305-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Over the past three decades the reverberation mapping technique was used to measure the central regions of Active Galactic Nuclei (AGN), their size, velocity field, and the mass of the black hole in the center. This technique was used mainly in the optical with several studies in the UV. Reverberation mapping in the UV adds essential information to the AGN studies. This paper reviews these recent studies done in the UV, presents results from the recent HST campaign toward NGC 5548, and discuss two projects of reverberation mapping of UV emission lines in high-luminosity quasars. The advantages of reverberation mapping in the UV will be discussed as well as the needs from new UV missions in order to be able to advance UV reverberation mapping campaigns.

引用

页数：8

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