2015/03/28 by Jiayi Sun, Yue Shen · 59 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Black hole (networking) #Dispersion (optics) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Luminosity #Quasar #Sequence (biology) #Sky #Spectral line #Velocity dispersion #astro-ph.GA
paper · pdf · doi:10.1088/2041-8205/804/1/l15
published in The Astrophysical Journal Letters 804(1), L15 (IOP Publishing) · ApJL in press; 5 pages and 4 figures
arxiv created 2015/03/28 · openalex publication_date 2015/04/27 · arxiv updated 2015/06/24 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
The diverse properties of broad-line quasars appear to follow a well-defined main sequence along which the optical Fe ii strength increases. It has been suggested that this sequence is mainly driven by the Eddington ratio ( L / L Edd ) of the black hole (BH) accretion. Shen & Ho demonstrated with quasar clustering analysis that the average BH mass decreases with increasing Fe ii strength when quasar luminosity is fixed, consistent with this suggestion. Here we perform an independent test by measuring the stellar velocity dispersion σ * (hence, the BH mass via the M – σ * relation) from decomposed host spectra in low-redshift Sloan Digital Sky Survey quasars. We found that at fixed quasar luminosity, σ * systematically decreases with increasing Fe ii strength, confirming that the Eddington ratio increases with Fe ii strength. We also found that at fixed luminosity and Fe ii strength, there is little dependence of σ * on the broad H β FWHM. These new results reinforce the framework that the Eddington ratio and orientation govern most of the diversity seen in broad-line quasar properties.