Results 111 to 120 of about 426,951 (145)
A Catalog of High-confidence Very Metal-poor Stars from DESI Based on a Deep Learning Method
Very metal-poor (VMP; [Fe/H]
Chen Yang +6 more
doaj +1 more source
Modelling the evolution and nucleosynthesis of carbon-enhanced metal-poor stars [PDF]
We present the results of binary population simulations of carbon-enhanced metal-poor (CEMP) stars. We show that nitrogen and fluorine are useful tracers of the origin of CEMP stars, and conclude that the observed paucity of very nitrogen-rich stars puts
Lugaro, Maria +3 more
core +1 more source
In this work, we present high-resolution ( R ∼ 100,000), high signal-to-noise ratio (S/N ∼ 800) spectroscopic observations for the well-known, bright, extremely metal-poor, carbon-enhanced star BD+44°493.
Vinicius M. Placco +13 more
doaj +1 more source
Near-Infrared Spectroscopy of Carbon-Enhanced Metal-Poor Stars. I. A SOAR/OSIRIS Pilot Study
International audienceWe report on an abundance analysis for a pilot study of seven carbon-enhanced metal-poor (CEMP) stars, based on medium-resolution optical and near-infrared spectroscopy. The optical spectra are used to estimate [Fe/H], [C/Fe], [N/Fe]
Lee, Youngsun +11 more
core +1 more source
In this work, we present high-resolution spectroscopic observations for six metal-poor stars with [Fe/H] < –3 (including one with [Fe/H] < –4), selected using narrowband Ca ii HK photometry from the DECam MAGIC Survey.
Vinicius M. Placco +24 more
doaj +1 more source
We present the discovery of HE 0144−4657, an ultra-metal-poor, CNO-enhanced star dynamically associated with the Helmi Stream disrupted dwarf-galaxy remnant.
Vinicius M. Placco +3 more
doaj +1 more source
Possibility of Secondary i- and s-processes Following r-process in the Collapsar Jet
The slow and intermediate neutron-capture processes, s - and i -processes, are believed to occur in asymptotic giant branch stars to provide half of the heavy atomic nuclei with A ≥ 90. We suggest a possibility that certain types of outflows found in the
Zhenyu He +7 more
doaj +1 more source
How Population III Supernovae Determined the Properties of the First Galaxies
Massive Population III stars can die as energetic supernovae that enrich the early Universe with metals and determine the properties of the first galaxies.
Ke-Jung Chen +6 more
doaj +1 more source
Tooth-Supporting Hard Tissue Regeneration Using Biopolymeric Material Fabrication Strategies. [PDF]
Kim MG, Park CH.
europepmc +1 more source
Near-infrared Observations of BD+44°493 with IGRINS-2
We present high-resolution ( ${ \mathcal R }\sim 45,000$ ), high-signal-to-noise (S/N > 200) H - and K -band spectra of BD+44°493 obtained with the newly commissioned IGRINS-2 instrument on the Gemini North Telescope.
Vinicius M. Placco, William D. Vacca
doaj +1 more source

