Annual Review of Astronomy and Astrophysics

By A. R. Rao. 2015

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Construction and physical properties of Kerr black holes with scalar hair (2015, background): “BH candidates of this type have been found within a mass range between 10(6) and 10(10) M [4] and they are thought to play a central role in both the formation and growth of their host galaxies [5]; thus understanding them is of vital importance for the models of structure formation in the Universe.”
Accretion into the central cavity of a circumbinary disc (2012, methodology): “The analytic solution assuming a constant coefficient of kinematic viscosity is well known and given by Pringle (1981).”
The CO-to-H2 Conversion Factor (2013, methodology): “A discussion of the results of older analyses can be found in Bloemen (1989), here we will refer to a few of the more recent results using the Compton Gamma Ray Observatory and Fermi satellites. Strong & Mattox (1996) analyzed the EGRET all-sky survey obtaining XCO,20 ≈ 1.9±0.2. Similar results were”