activity
19982009
most citedNear-UV Observations of HD221170: New Insights into the Nature of r-Process-Rich Stars

241 citations · 1.1k across the 18 of their papers we have counts for

collaborators
Showing 2009Show all

5 papers · 1 filter

astro-ph.SR2009152 cited

Improved Laboratory Transition Probabilities for Ce II, Application to the Cerium Abundances of the Sun and Five r-process Rich, Metal-Poor Stars, and Rare Earth Lab Data

J. E. Lawler, C. Sneden, J. J. Cowan +2

Recent radiative lifetime measurements accurate to +/- 5% using laser-induced fluorescence (LIF) on 43 even-parity and 15 odd-parity levels of Ce II have been combined with new bra…

astro-ph.SR2009208 cited

New Rare Earth Element Abundance Distributions for the Sun and Five r-Process-Rich Very Metal-Poor Stars

Christopher Sneden, James E. Lawler, John J. Cowan +2

We have derived new abundances of the rare-earth elements Pr, Dy, Tm, Yb, and Lu for the solar photosphere and for five very metal-poor, neutron-capture r-process-rich giant stars.…

astro-ph.IM2009

New Discoveries in Planetary Systems and Star Formation through Advances in Laboratory Astrophysics

AAS WGLA, Nancy Brickhouse, John Cowan +9

As the panel on Planetary Systems and Star Formation (PSF) is fully aware, the next decade will see major advances in our understanding of these areas of research. To quote from th…

astro-ph.IM2009

New Discoveries in the Galactic Neighborhood through Advances in Laboratory Astrophysics

AAS WGLA, Nancy Brickhouse, John Cowan +9

As the Galactic Neighborhood (GAN) panel is fully aware, the next decade will see major advances in our understanding of this area of research. To quote from their charge, these ad…

astro-ph.SR2009101 cited

Nucleosynthesis Modes in the High-Entropy-Wind of Type II Supernovae: Comparison of Calculations with Halo-Star Observations

K. Farouqi, K. -L. Kratz, L. I. Mashonkina +4

While the high-entropy wind (HEW) of Type II supernovae remains one of the more promising sites for the rapid neutron-capture (r-) process, hydrodynamic simulations have yet to rep…