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The Accretion and Obscured Growth of Supermassive Black Holes - First Constraints on the Local Heavily Obscured AGN Fraction with NuSTAR (Hardcover, 1st ed. 2021)
Loot Price: R4,510
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The Accretion and Obscured Growth of Supermassive Black Holes - First Constraints on the Local Heavily Obscured AGN Fraction with NuSTAR (Hardcover, 1st ed. 2021)
Series: Springer Theses
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This thesis describes the application of state-of-the-art
high-energy X-ray studies to the astronomical quest for
understanding obscured active galactic nuclei (AGN). These AGN are
supermassive black holes growing by accretion of matter located in
the nuclei of galaxies. The material that feeds these black holes
also obscures them from view, rendering them challenging to study.
It is possible to study them by effectively 'X-raying' galactic
nuclei to peer through these obscuring veils. Beginning with the
proof-of-concept application of novel X-ray Monte Carlo codes to
the Nuclear Spectroscopic Telescope ARray (NuSTAR) spectrum of a
known heavily obscured AGN, the thesis establishes the relevant
parameters that characterise the AGN spectrum and central black
hole growth rate. Next the largest sample of known heavily obscured
AGN is compiled, finding the strength of a prominent iron spectral
feature to weaken with AGN power. This is puzzling, and suggests
that there may be more hidden AGN than previously thought. Finally
by combining an all-sky infrared selection with NuSTAR follow-up,
new heavily obscured AGN are identified. Obscuration emits infrared
radiation, meaning that the infrared-selected AGN catalogue should
be representative of the underlying AGN population. The absence of
such representative catalogues has continually plagued cosmological
studies, and the resultant obscured AGN fraction will be strongly
constraining for AGN models.
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