2015AJ....149...85G -
Astron. J., 149, 85 (2015/February-0)
Is there a connection between broad absorption line quasars and narrow-line Seyfert 1 galaxies?
GRUPE D. and NOUSEK J.A.
Abstract (from CDS):
We consider whether broad absorption line quasars (BAL QSOs) and narrow-line Seyfert 1 galaxies (NLS1s) are similar, as suggested by Brandt & Gallagher and Boroson. For this purpose, we constructed a sample of 11 BAL QSOs from existing Chandra and Swift observations. We found that BAL QSOs and NLS1s both operate at high Eddington ratios L/LEdd, although BAL QSOs have slightly lower L/LEdd. BAL QSOs and NLS1s in general have high Fe ii/Hβ and low [O iii]/Hβ ratios following the classic "Boroson & Green" eigenvector 1 relation. We also found that the mass accretion rates {dot}M of BAL QSOs and NLS1s are more similar than previously thought, although some BAL QSOs exhibit extreme mass accretion rates of more than 10 M☉yr. These extreme mass accretion rates may suggest that the black holes in BAL QSOs are relativistically spinning. Black hole masses in BAL QSOs are a factor of 100 larger than NLS1s. From their location on a M - σ plot, we find that BAL QSOs contain fully developed black holes. Applying a principal component analysis to our sample, we find eigenvector 1 to correspond to the Eddington ratio L/LEdd, and eigenvector 2 to black hole mass.
Abstract Copyright:
∼
Journal keyword(s):
galaxies: active
CDS comments:
SDSS J143748+432707 is a probable misprint for SDSS J143748.28-014710.7.
Simbad objects:
33
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