activity
20072023
most citedSingle and binary evolution of Population III stars and their supernovae light curves

16 citations · 27 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2023

Evolution of low mass population III stars from the pre-main sequence to the white dwarf cooling track

T. M. Lawlor, J. MacDonald

Radiation feedback from massive population III stars may have given rise to low mass star formation from primordial or nearly primordial material. If early universe low mass stars…

astro-ph.SR2023

A closer look at low mass post-AGB late thermal pulses

Timothy M. Lawlor

Thermal Pulse (LTP) stellar evolution models experience a helium pulse that occurs following Asymptotic Giant Branch (AGB) departure and causes a rapid looping evolution in the HR…

astro-ph.SR2021★ 6 cited

New models for the rapid evolution of the central star of the Stingray Nebula

Timothy M. Lawlor

We present stellar evolution calculations from the Asymptotic Giant Branch (AGB) to the Planetary Nebula (PN) phase for models of initial mass 1.2 M\odot and 2.0 M\odot that experi…

astro-ph.SR2015★ 5 cited

The effects of convection criteria on the evolution of population III stars and the detectability of their supernovae

T. M. Lawlor, T. R. Young, J. Teffs +1

The first stars continue to elude modern telescopes, but much has been accomplished in observing the glow of the first galaxies. As detection capabilities improve we will eventuall…

astro-ph2007★ 16 cited

Single and binary evolution of Population III stars and their supernovae light curves

T. M. Lawlor, T. R. Young, T. A. Johnson +1

We present stellar evolution calculations for Population III stars for both single and binary star evolution. Our models include 10 Msun and 16.5 Msun single stars and a 10 Msun mo…