Two-component structure of the hβ broad-line region in quasars. I. evidence from spectral principal component analysis

Chen Hu, Jian Min Wang, Luis C. Ho, Gary J. Ferland, Jack A. Baldwin, Ye Wang

Research output: Contribution to journalArticlepeer-review

26 Scopus citations

Abstract

We report on a spectral principal component analysis (SPCA) of a sample of 816 quasars, selected to have small Fe II velocity shifts with spectral coverage in the rest wavelength range 3500-5500 Å. The sample is explicitly designed to mitigate spurious effects on SPCA induced by Fe II velocity shifts. We improve the algorithm of SPCA in the literature and introduce a new quantity, the fractional-contribution spectrum, that effectively identifies the emission features encoded in each eigenspectrum. The first eigenspectrum clearly records the power-law continuum and very broad Balmer emission lines. Narrow emission lines dominate the second eigenspectrum. The third eigenspectrum represents the Fe II emission and a component of the Balmer lines with kinematically similar intermediate-velocity widths. Correlations between the weights of the eigenspectra and parametric measurements of line strength and continuum slope confirm the above interpretation for the eigenspectra. Monte Carlo simulations demonstrate the validity of our method to recognize cross talk in SPCA and firmly rule out a single-component model for broad Hβ. We also present the results of SPCA for four other samples that contain quasars in bins of larger Fe II velocity shift; similar eigenspectra are obtained. We propose that the Hβ-emitting region has two kinematically distinct components: one with very large velocities whose strength correlates with the continuum shape and another with more modest, intermediate velocities that is closely coupled to the gas that gives rise to Fe II emission.

Original languageEnglish
Article number126
JournalAstrophysical Journal
Volume760
Issue number2
DOIs
StatePublished - Dec 1 2012

Keywords

  • line: profiles
  • methods: data analysis
  • methods: numerical
  • methods: statistical
  • quasars: emission lines
  • quasars: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Two-component structure of the hβ broad-line region in quasars. I. evidence from spectral principal component analysis'. Together they form a unique fingerprint.

Cite this