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Article Dans Une Revue Research in Astronomy and Astrophysics Année : 2014

A search for double-peaked narrow emission line galaxies and AGNs in the LAMOST DR1

Zhi-Xin Shi
  • Fonction : Auteur
A-Li Luo
  • Fonction : Auteur
Xiao-Yan Chen
  • Fonction : Auteur
Peng Wei
  • Fonction : Auteur
Yong-Heng Zhao
  • Fonction : Auteur
Fu-Chao Wu
  • Fonction : Auteur
Yan-Xia Zhang
  • Fonction : Auteur
Shi-Yin Shen
  • Fonction : Auteur
Hong Wu
  • Fonction : Auteur
Xue-Bing Wu
  • Fonction : Auteur
Hao-Tong Zhang
  • Fonction : Auteur
Ya-Juan Lei
  • Fonction : Auteur
Jian-Nan Zhang
  • Fonction : Auteur
Ting-Gui Wang
  • Fonction : Auteur
Ge Jin
  • Fonction : Auteur
Yong Zhang

Résumé

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) has released more than two million spectra, which provide the opportunity to search for double-peaked narrow emission line (NEL) galaxies and active galactic nuclei (AGNs). The double-peaked narrow-line profiles can be well modeled by two velocity components, respectively blueshifted and redshifted with respect to the systemic recession velocity. This paper presents 20 double-peaked NEL galaxies and AGNs found from LAMOST DR1 using a search method based on a multi-Gaussian fit of the narrow emission lines. Among them, ten have already been published by other authors, either listed as genuine double-peaked NEL objects or as asymmetric NEL objects, and the remaining ten are original discoveries. We discuss some possible origins for the double-peaked narrow-line features, such as interaction between jet and narrow line regions, interaction with companion galaxies, and black hole binaries. Spatially resolved optical imaging and/ or follow-up observations in other spectral bands are needed to further discuss the physical mechanisms at work.

Dates et versions

hal-01441976 , version 1 (20-01-2017)

Identifiants

Citer

Zhi-Xin Shi, A-Li Luo, Georges Comte, Xiao-Yan Chen, Peng Wei, et al.. A search for double-peaked narrow emission line galaxies and AGNs in the LAMOST DR1. Research in Astronomy and Astrophysics, 2014, 14 (10), pp.1234--1250. ⟨10.1088/1674-4527/14/10/003⟩. ⟨hal-01441976⟩
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