Spectral changes and BLR kinematics of eruptive changing-look AGN

被引：4

作者：

Ochmann, M. W. ^{[1
]}

Kollatschny, W. ^{[1
]}

Zetzl, M. ^{[1
]}

机构：

[1] Univ Gottingen, Inst Astrophys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany

来源：

CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO | 2020年 / 50卷 / 01期

关键词：

active galactic nuclei; changing-look; broad line region; accretion disk; spectroscopy; HE1136-2304; NGC1566; EMISSION-LINE VARIABILITY; REGION;

D O I：

10.31577/caosp.2020.50.1.318

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present results of recent optical spectroscopic variability campaigns for HE1136-2304 and NGC1566 which exhibited X-ray outbursts in July 2014 and June 2018, respectively. We show that the broad line region (BLR) structure in the changing-look AGN HE1136-2304 is similar to that of non-changing-look AGN and that the BLR kinematics is dominated by Keplerian accretion disk (AD) rotation. Furthermore, we present an optical spectrum of NGC1566 taken only a few weeks after its X-ray outburst, clearly showing drastic spectral changes.

引用

页码：318 / 327

页数：10

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