Blue outliers among intermediate redshift quasars

被引：23

作者：

Marziani, P. ^{[1
]}

Sulentic, J. W. ^{[2
]}

Stirpe, G. M. ^{[3
]}

Dultzin, D. ^{[4
]}

Del Olmo, A. ^{[5
]}

Martinez-Carballo, M. A. ^{[5
]}

机构：

[1] Osserv Astron Padova, INAF, Padua, Italy

[2] CSIC, Inst Astrofis Andalucia, Granada, Spain

[3] Osservatorio Astron Bologna, INAF, Bologna, Italy

[4] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City, DF, Mexico

[5] CSIC, Inst Astrofis Andalucia, Granada, Spain

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2016年 / 361卷 / 01期

关键词：

Galaxies: active; Quasars: emission lines; Quasars: general; Techniques: spectroscopic; Astronomical databases: surveys; ACTIVE GALACTIC NUCLEI; NARROW-LINE REGIONS; NEAR-INFRARED SPECTROSCOPY; BLACK-HOLE MASS; H-BETA REGION; EMISSION-LINE; SEYFERT-GALAXIES; VLT/ISAAC SPECTRA; SAMPLE; STELLAR;

D O I：

10.1007/s10509-015-2590-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

[OIII]lambda 5007 "blue outliers"-that are suggestive of outflows in the narrow line region of quasars-appear to be much more common at intermediate z (high luminosity) than at low z. About 40 % of quasars in a Hamburg ESO intermediate z sample of 52 sources qualify as "blue outliers" (i.e., quasars with [OIII]lambda lambda 4959, 5007 lines showing large systematic blueshifts with respect to rest frame). We discuss major findings on what has become an intriguing field in active galactic nuclei research and stress the relevance of "blue outliers" to feedback and host galaxy evolution.

引用

页码：1 / 10

页数：10

共 65 条

[51] NO EVIDENCE FOR A SYSTEMATIC Fe II EMISSION LINE REDSHIFT IN TYPE 1 ACTIVE GALACTIC NUCLEI [J].