Pagan and Christian in an Age of Anxiety. By E. R. Dodds. Cambridge: At the University Press, 1965. 144 pp. $5.50.

Schoedel, William R.

doi:10.2307/3162675

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Astrophysical Uncertainties1

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2007

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“…Density profiles of galactic nuclei.-Direct observational constraints on the stellar density within the sphere of influence of MBHs with masses in the LISA range exist only for the Milky Way [4,85,119,122,123,199,206,251,283] and M 32 [188]. Even in these cases the interpretation of the (projected) surface brightness or number counts in terms of stellar density is a difficult and uncertain matter, mostly because these observations are dominated by bright stars whose distribution probably does not trace that of the compact remnants [5].…”

Section: Astrophysical Uncertaintiesmentioning

confidence: 99%

Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA

Amaro-Seoane¹,

Gair²,

Freitag³

et al. 2007

Class. Quantum Grav.

537

634

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Black hole binaries with extreme ( 10 4 : 1) or intermediate (∼10 2 -10 4 : 1) mass ratios are among the most interesting gravitational wave sources that are expected to be detected by the proposed laser interferometer space antenna (LISA). These sources have the potential to tell us much about astrophysics, but are also of unique importance for testing aspects of the general theory of relativity in the strong field regime. Here we discuss these sources from the perspectives of astrophysics, data analysis and applications to testing general relativity, providing both a description of the current state of knowledge and an outline of some of the outstanding questions that still need to be addressed.

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