output
20012026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2017 · astro-ph.SRShow all

14 papers · 2 filters

astro-ph.SR2017★ 43 cited

The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors

C. E. Fields, F. X. Timmes, R. Farmer +3

We explore properties of core-collapse supernova progenitors with respect to the composite uncertainties in the thermonuclear reaction rates by coupling the reaction rate probabili…

astro-ph.SR2017★ 36 cited

Convective boundary mixing in a post-He core burning massive star model

Austin Davis, Sam Jones, Falk Herwig

Convective boundary mixing (CBM) in the advanced evolutionary stages of massive stars is not well understood. Structural changes caused by convection have an impact on the evolutio…

astro-ph.SR2017★ 88 cited

Pop III -process Nucleosynthesis and the Elemental Abundances of SMSS J0313-6708 and the Most Iron-Poor Stars

O. Clarkson, F. Herwig, M. Pignatari

We have investigated a highly energetic H-ingestion event during shell He burning leading to H-burning luminosities of $\log(L_\mathrm{H}/\mathrm{\Lsun}) \sim 13$ in a $45 \Msun$ P…

astro-ph.SR2017★ 146 cited

JINAbase: A database for chemical abundances of metal-poor stars

Abdu Abohalima, Anna Frebel

Reconstructing the chemical evolution of the Milky Way is crucial for understanding the formation of stars, planets, and galaxies throughout cosmic time. Different studies associat…

astro-ph.SR2017★ 178 cited

NuGrid Stellar Data Set. II. Stellar Yields from H to Bi for Stellar Models with Mzams = 1 to 25Msun and Z = 0.0001 to 0.02

C. Ritter, F. Herwig, S. Jones +3

We provide here a significant extension of the NuGrid Set 1 models in mass coverage and toward lower metallicity, adopting the same physics assumptions. The combined data set now i…

astro-ph.SR2017★ 21 cited

Neutron-capture element abundances in the planetary nebula NGC 5315 from deep optical and near-infrared spectrophotometry

S. Madonna, J. García-Rojas, N. C. Sterling +5

We analyze the chemical composition of the planetary nebula (PN) NGC 5315, through high-resolution (R = 40000) optical spectroscopy with UVES at the Very Large Telescope, and mediu…