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20012003
most citedMassive black hole remnants of the first stars in galactic haloes

89 citations · 206 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2003★ 27 cited

Massive black hole remnants of the first stars III: observational signatures from the past

Ranty R. Islam, James E. Taylor, Joseph Silk

The first stars forming in minihaloes at redshifts greater than 20 may have been very massive and could have left behind massive black hole (MBH) remnants. In previous papers we in…

astro-ph2003★ 22 cited

Massive black hole remnants of the first stars II: optical and X-ray signatures in present-day galactic haloes

Ranty R. Islam, James E. Taylor, Joseph Silk

The first stars forming in minihaloes at redshifts greater than 20 may have been very massive and could have left behind massive black hole (MBH) remnants. In a previous paper we i…

astro-ph2003★ 49 cited

Massive black hole remnants of the first stars I: abundance in present-day galactic haloes

Ranty R. Islam, James E. Taylor, Joseph Silk

We investigate the possibility that present-day galaxies and their dark matter haloes contain a population of massive black holes (MBHs) that form by hierarchical merging of the bl…

astro-ph2002

Non-Standard Structure Formation Scenarios

Alexander Knebe, Brett Little, Ranty Islam +3

Observations on galactic scales seem to be in contradiction with recent high resolution N-body simulations. This so-called cold dark matter (CDM) crisis has been addressed in sever…

astro-ph2002★ 89 cited

Massive black hole remnants of the first stars in galactic haloes

Ranty R. Islam, James E. Taylor, Joseph Silk

We investigate the possibility that present-day galactic haloes contain a population of massive black holes (MBHs) that form by hierarchical merging of the black hole remnants of t…

astro-ph2002★ 5 cited

Warm Dark Matter versus Bumpy Power Spectra

Brett Little, Alexander Knebe, Ranty Islam

In this paper we are exploring the differences between a Warm Dark Matter model and a CDM model where the power on a certain scale is reduced by introducing a narrow negative featu…