activity
19972000
most citedThe profile and equivalent width of the X-ray iron emission-line from a disk around a Kerr black hole

154 citations · 235 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph2000★ 42 cited

Reflected Iron Line From a Source Above a Kerr Black Hole Accretion Disc

Y. Dabrowski, A. N. Lasenby

In this paper we present a fully relativistic approach to modelling both the continuum emission and the reflected fluorescent iron line from a primary X-ray source near a Kerr blac…

astro-ph1999★ 3 cited

Microwave background anisotropies due to non-linear structures in open and Lambda universes

Y. Dabrowski, M. J. Hall, I. L. Sawicki +1

A new method arising from a gauge-theoretic approach to general relativity is applied to the formation of clusters in an expanding universe. The three cosmological models (Omega_0=…

astro-ph1998

Spinning Black Holes in Active Galactic Nuclei

Y. Dabrowski

Recent X-ray spectroscopy made with ASCA have shown broad, skewed iron line emission from Seyfert-1 galaxies. The large extent of the red tail allows probing of the innermost regio…

astro-ph1998★ 4 cited

Review of Ground-Based CMB Experiments

A. N. Lasenby, A. W. Jones, Y. Dabrowski

We present in this paper a brief review of Ground-Based Cosmic Microwave Background (CMB) experiments. We first recall the main experimental problems and adopted solutions. We then…

astro-ph1998★ 13 cited

Microwave background anisotropies and non-linear structures II. Numerical computations

Y. Dabrowski, M. P. Hobson, A. N. Lasenby +1

A new method for modelling spherically symmetric inhomogeneities is applied to the formation of clusters in an expanding Universe. We impose simple initial velocity and density per…

astro-ph1998★ 11 cited

Microwave Background Anisotropies and Nonlinear Structures I. Improved Theoretical Models

A. N. Lasenby, C. J. L. Doran, M. P. Hobson +2

A new method is proposed for modelling spherically symmetric inhomogeneities in the Universe. The inhomogeneities have finite size and are compensated, so they do not exert any mea…