喵ID：6X14yw
Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence
Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence
Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence来自两年高节奏混响测绘活动的类星体 PG 2130 099 的宽线区域
基本信息
DOI：
10.3847/1538-4357/ab6a17
10.3847/1538-4357/ab6a17发表时间：
2020-01
2020-01期刊：
The Astrophysical Journal
The Astrophysical Journal影响因子：
--
--通讯作者：
Wang Jian-Min
Wang Jian-Min中科院分区：
其他
其他文献类型：
--
-- 作者： Hu Chen;Li Yan-Rong;Du Pu;Zhang Zhi-Xiang;Li Sha-Sha;Huang Ying-Ke;Lu Kai-Xing;Bai Jin-Ming;Ho Luis C.;Bian Wei-Hao;Brotherton Michael S.;Yuan Ye-Fei;Aceituno Jesus;Winkler Hartmut;Wang Jian-Min
研究方向： --
MeSH主题词： --
关键词： --
来源链接：pubmed详情页地址
文献摘要
As one of the most interesting Seyfert 1 galaxies, PG 2130+099 has been the target of several reverberation mapping (RM) campaigns over the years. However, its measured broad Hβ line responses have been inconsistent, with time lags of ∼200 days, ∼25 days,
作为最有趣的赛弗特1型星系之一，PG 2130 + 099多年来一直是若干反响映射（RM）活动的目标。然而，其测量到的宽Hβ线响应一直不一致，时间延迟约为200天、约25天。
参考文献（63）
被引文献（10）
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2012-06
2012-06影响因子：
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1988-09
1988-09影响因子：
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2013-05影响因子：
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C. Grier;P. Martini;L. Watson;B. Peterson;M. Bentz;K. Dasyra;M. Dietrich;L. Ferrarese;R. Pogge;Y. Zu通讯作者：
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10.1088/0004-637x/718/1/460发表时间：
2010-05
2010-05影响因子：
0
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W. Bian;K. Huang;Chen Hu;Li Zhang;Q. Yuan;Ke-liang Huang;Jian-Min Wang
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10.1086/420755发表时间：
2002-01
2002-01影响因子：
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K. Horne;B. Peterson;S. Collier;H. Netzer通讯作者：
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