Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Supplemental Material

@article{Kormendy2013CoevolutionN,
  title={Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Supplemental Material},
  author={J. Kormendy and L. Ho},
  journal={arXiv: Cosmology and Nongalactic Astrophysics},
  year={2013}
}
  • J. Kormendy, L. Ho
  • Published 2013
  • Physics
  • arXiv: Cosmology and Nongalactic Astrophysics
  • This is the Supplemental Material to Kormendy and Ho 2013, ARAA, 51, 511 (arXiv:1304.7762). Section S1 summarizes indirect methods that are used to estimate black hole (BH) masses for galaxies with active nuclei (AGNs). Section S2 lists the observational criteria that are used to classify classical and pseudo bulges. The (pseudo)bulge classifications used in the main paper are not based on physical interpretation; rather, they are based on these observational criteria. Section S3 supplements… CONTINUE READING
    Ultralight scalars as cosmological dark matter
    • 495
    • PDF
    The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
    • 378
    • Highly Influenced
    • PDF
    The Illustris simulation: the evolving population of black holes across cosmic time
    • 253
    • Highly Influenced
    • PDF
    THE BLACK HOLE-BULGE MASS RELATION in MEGAMASER HOST GALAXIES
    • 36
    • Highly Influenced
    • PDF
    A ∼50,000 M⊙ SOLAR MASS BLACK HOLE IN THE NUCLEUS OF RGG 118
    • 95
    • Highly Influenced
    • PDF
    The diversity of quasars unified by accretion and orientation
    • 150
    • PDF

    References

    Publications referenced by this paper.
    SHOWING 1-10 OF 759 REFERENCES
    Formation of supermassive black holes
    • 379
    • PDF