activity
19952015
most citedThe theoretical instability strip of M dwarf stars

23 citations · 82 across the 6 of their papers we have counts for

collaborators

6 papers

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-ph.SR2014★ 14 cited

M dwarf search for pulsations within Kepler GO program

C. Rodríguez-López, J. E. Gizis, J. MacDonald +2

We present the analysis of four M dwarf stars -plus one M giant that seeped past our selection criteria- observed in Cycle 3 of Kepler Guest Observer program (GO3) in a search for…

astro-ph.SR2013★ 23 cited

The theoretical instability strip of M dwarf stars

C. Rodríguez-López, J. MacDonald, P. J. Amado +2

The overstability of the fundamental radial mode in M dwarf models was theoretically predicted by Rodríguez-López et al. (2012). The periods were found to be in the ranges ~25-40 m…

astro-ph.SR2013★ 11 cited

The extremely low metallicity star SDSS J102915+172927: a subgiant scenario

J. MacDonald, T. M. Lawlor, N. Anilmis +1

Spectroscopic analysis of the Galactic halo star SDSS J102915+172927 has shown it to have a very low heavy element abundance, Z < 7.4 10-7, with [Fe/H] = -4.89 plus/minus 0.10 and…

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…

astro-ph1995★ 13 cited

Stellar evolution with mass loss - comparison of numerical and semi-analytical computations.

R. Jimenez, U. G. Jorgensen, P. Thejll +2

We present here results of stellar evolution calculations that include the latest advances in radiative opacities and neutrino cooling, and discuss on the basis of these models how…