John Eldridge
www.mendeley.com
0000-0002-1722-6343
University of Auckland
90 papers found
Refreshing results…
On aging star clusters using red supergiants independent of the fraction of interacting binary stars.
The uncertain masses of progenitors of core-collapse supernovae and direct-collapse black holes
Dependence of gravitational wave transient rates on cosmic star formation and metallicity evolution history
Binary population synthesis models for core-collapse gamma-ray burst progenitors
The 50–100 pc scale parent stellar populations of Type II supernovae and limitations of single star evolution models
Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow
The distance, supernova rate, and supernova progenitors of NGC 6946
Impact of binary interaction on the evolution of blue supergiants
Initial mass function variations cannot explain the ionizing spectrum of low metallicity starbursts
Supernova lightCURVE POPulation Synthesis II: Validation against supernovae with an observed progenitor
On the Chirp Mass Distribution of Stellar Origin Gravitational-wave Events
Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations
A consistent estimate for gravitational wave and electromagnetic transient rates
Neutron star kicks – II. Revision and further testing of the conservation of momentum ‘kick’ model
Re-evaluating old stellar populations
How fast can stellar death throes go?
Emission-line diagnostics of nearby H ii regions including interacting binary populations
Observational properties of massive black hole binary progenitors
Supernova lightCURVE POPulation Synthesis I: Including interacting binaries is key to understanding the diversity of type II supernova lightcurves
Spatially Resolved MaNGA Observations of the Host Galaxy of Superluminous Supernova 2017egm
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