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Properties of active galaxies at the extreme of eigenvector 1

文献类型:期刊论文

作者Sniegowska, M.1,2; Czerny, B.1; You, B.3,4; Panda, S.1,3; Wang, J. -M.5; Hryniewicz, K.3; Wildy, C.1
刊名Astronomy & astrophysics
出版日期2018-05-28
卷号613页码:12
ISSN号1432-0746
关键词Quasars: emission lines Accretion, accretion disks
DOI10.1051/0004-6361/201730433
通讯作者Czerny, b.(bcz@camk.edu.pl)
英文摘要Context. eigenvector 1 (ev1) is the formal parameter which allows the introduction of some order in the properties of the unobscured type 1 active galaxies. aims. we aim to understand the nature of this parameter by analyzing the most extreme examples of quasars with the highest possible values of the corresponding eigenvalues r-fe. methods. we selected the appropriate sources from the sloan digital sky survey (sdss) and performed detailed modeling, including various templates for the fe ii pseudo-continuum and the starlight contribution to the spectrum. results. out of 27 sources with r-fe larger than 1.3 and with the measurement errors smaller than 20% selected from the sdss quasar catalog, only six sources were confirmed to have a high value of r-fe, defined as being above 1.3. all other sources have an r-fe of approximately 1. three of the high r-fe objects have a very narrow h beta line, below 2100 km s(-1) but three sources have broad lines, above 4500 km s(-1), that do not seem to form a uniform group, differing considerably in black hole mass and eddington ratio; they simply have a very similar ew([oiii]5007) line. therefore, the interpretation of the ev1 remains an open issue.
WOS关键词DIGITAL SKY SURVEY ; EMISSION-LINE PROPERTIES ; FE-II EMISSION ; GALACTIC NUCLEI ; BLACK-HOLE ; CORRELATION SPACE ; QUASAR SPECTRA ; SAMPLE ; EXTINCTION ; ACCRETION
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
语种英语
出版者EDP SCIENCES S A
WOS记录号WOS:000433276100001
URI标识http://www.irgrid.ac.cn/handle/1471x/2177517
专题高能物理研究所
通讯作者Czerny, B.
作者单位1.Polish Acad Sci, Ctr Theoret Phys, Al Lotnikow 32-46, PL-02668 Warsaw, Poland
2.Univ Warsaw Observ, Al Ujazdowskie 4, PL-00478 Warsaw, Poland
3.Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland
4.Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China
5.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, 19B Yuquan Rd, Beijing 100049, Peoples R China
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GB/T 7714
Sniegowska, M.,Czerny, B.,You, B.,et al. Properties of active galaxies at the extreme of eigenvector 1[J]. Astronomy & astrophysics,2018,613:12.
APA Sniegowska, M..,Czerny, B..,You, B..,Panda, S..,Wang, J. -M..,...&Wildy, C..(2018).Properties of active galaxies at the extreme of eigenvector 1.Astronomy & astrophysics,613,12.
MLA Sniegowska, M.,et al."Properties of active galaxies at the extreme of eigenvector 1".Astronomy & astrophysics 613(2018):12.

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来源:高能物理研究所

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