The origin of weak emission-line AGNs

Yuan Liu*, Jin Zhang, Shuang Nan Zhang

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Some abnormal AGNs are discovered in the SDSS data recently. The usual UV/optical emission lines are exceptionally weak in their UV/optical spectroscopy, though the shapes and luminosities of their continua are comparable with that of the normal AGNs. We investigated the optical variations and the near-infrared spectra of these weak emission-line AGNs. We propose that these AGNs can be interpreted as the early stage of an active cycle of AGNs.

Original languageEnglish
Title of host publicationFeeding Compact Objects
Subtitle of host publicationAccretion on All Scales
EditorsChengmin Zhang, Tomaso Belloni, Mariano Mendez, Shuangnan Zhang
Pages267-268
Number of pages2
EditionS290
DOIs
Publication statusPublished - Aug 2012
Externally publishedYes

Publication series

NameProceedings of the International Astronomical Union
NumberS290
Volume8
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • Quasars: emission lines
  • infrared: galaxies
  • line: formation

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