activity
19992009
most citedThe spin and shape of dark matter haloes in the Millennium simulation of a LambdaCDM universe

488 citations · 1.5k across the 22 of their papers we have counts for

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Showing 2008Show all

12 papers · 1 filter

astro-ph200811 cited

A multi-wavelength survey of AGN in the XMM-LSS field: I. Quasar selection via the KX technique

Th. Nakos, J. P. Willis, S. Andreon +16

AIMS: We present a sample of candidate quasars selected using the KX-technique. The data cover 0.68 deg^2 of the X-ray Multi-Mirror (XMM) Large-Scale Structure (LSS) survey area wh…

astro-ph2008

Complete nucleosynthesis calculations for low-mass stars from NuGrid

Marco Pignatari, Falk Herwig, Michael Bennett +8

Many nucleosynthesis and mixing processes of low-mass stars as they evolve from the Main Sequence to the thermal-pulse Asymptotic Giant Branch phase (TP-AGB) are well understood (a…

astro-ph20083 cited

Spatial Distribution of Nucleosynthesis Products in Cassiopeia A: Comparison Between Observations and 3D Explosion Models

Patrick Young, Carola I. Ellinger, Francis X. Timmes +10

We examine observed heavy element abundances in the Cassiopeia A supernova remnant as a constraint on the nature of the Cas A supernova. We compare bulk abundances from 1D and 3D e…

astro-ph2008

NuGrid: s process in massive stars

Raphael Hirschi, Urs Frischknecht, F. -K. Thielemann +10

The s-process production in massive stars at very low metallicities is expected to be negligible due to the low abundance of the neutron source 22Ne, to primary neutron poisons and…

astro-ph2008

Nucleosynthesis simulations for a wide range of nuclear production sites from NuGrid

Falk Herwig, Michael Bennett, Steven Diehl +8

Simulations of nucleosynthesis in astrophysical environments are at the intersection of nuclear physics reaction rate research and astrophysical applications, for example in the ar…

astro-ph2008

44Ti and 56Ni in core-collapse supernovae

Georgios Magkotsios, Francis X. Timmes, Michael Wiescher +9

We investigate the physical conditions where 44Ti and 56Ni are created in core-collapse supernovae. In this preliminary work we use a series of post-processing network calculations…