output
19982026
most citedRotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones

888 citations

Showing 2006Show all

9 papers · 1 filter

astro-ph2006★ 57 cited

Mass loss and yield uncertainty in low-mass asymptotic giant branch stars

Richard J. Stancliffe, C. Simon Jeffery

We investigate the uncertainty in surface abundances and yields of asymptotic giant branch (AGB) stars. We apply three different mass loss laws to a 1.5 solar mass star of metallic…

astro-ph2006★ 158 cited

Rotational Modulation of the Radio Emission from the M9 Dwarf TVLM 513-46546: Broadband Coherent Emission at the Substellar Boundary?

G. Hallinan, A. Antonova, J. G. Doyle +3

The Very Large Array was used to observe the ultracool, rapidly rotating M9 dwarf TVLM 513-46546 simultaneously at 4.88 GHz and 8.44 GHz. The radio emission was determined to be pe…

astro-ph2006★ 43 cited

Stellar archaeology: the evolving spectrum of FG Sge

C. S. Jeffery, D. Schoenberner

Over an interval of 120 years, the extraordinary object FG Sge has been transformed from a hot post-AGB star to a very luminous cool supergiant. Theoretically, this evolution has b…

astro-ph2006★ 85 cited

Gravity-mode pulsations in subdwarf B stars: a critical test of stellar opacity

C. S. Jeffery, H. Saio

The identification of non-radial g-mode oscillations as the cause of variability in cool subdwarf B stars (PG1716 variables) has been frustrated by a 5 000 K discrepancy between th…

astro-ph2006★ 22 cited

On the angular momentum evolution of merged white dwarfs

K. N. Gourgouliatos, C. S. Jeffery

We study the angular momentum evolution of binaries containing two white dwarfs which merge and become cool helium-rich supergiants. Our object is to compare predicted rotation vel…

astro-ph2006★ 49 cited

Fe-bump instability: the excitation of pulsations in subdwarf B and other low-mass stars

C. S. Jeffery, H. Saio

We consider the excitation of radial and non-radial oscillations in low-mass B stars by the iron-bump opacity mechanism. The results are significant for the interpretation of pulsa…