Results 41 to 50 of about 167,710 (319)
Thermohaline Mixing in Extremely Metal-poor Stars [PDF]
Abstract Extremely metal-poor (EMP) stars are an integral piece in the puzzle that is the early universe, and although anomolous subclasses of EMP stars such as carbon-enhanced metal-poor (CEMP) stars are well studied, they make up less than half of all EMP stars with [Fe/H] ∼ −3.0.
Kate Henkel +4 more
openaire +2 more sources
In this work, we study the phase-space and chemical properties of the Sagittarius (Sgr) stream, the tidal tails produced by the ongoing destruction of the Sgr dwarf spheroidal (dSph) galaxy, focusing on its very metal-poor (VMP; [Fe/H] < −2) content.
Guilherme Limberg +8 more
doaj +1 more source
ABOUT THE HEAVY ELEMENTS ABUNDANCES IN THE ATMOSPHERES OF STARS WITH LOW METALLICITY
We present results of preliminary determinations of abundances of heavy elements in three metal-poor stars: HD37828, HD44008, HD221170. Careful comparison of observed and synthetic spectra permit us to increase the number of lines heavy elements ...
V. F. Gopka +3 more
doaj +1 more source
Massive first star binaries as new tools for Galactic archaeology [PDF]
Binary systems are important probes of the origin of stars with peculiar chemical features through the interactions between two stars. We have studied the evolution of a metal-free massive binary after the collision of the supernova ejecta with a low ...
Suda Takuma +4 more
doaj +1 more source
Very Metal-poor Stars in the Outer Galactic Bulge Found by the Apogee Survey [PDF]
Despite its importance for understanding the nature of early stellar generations and for constraining Galactic bulge formation models, at present little is known about the metal-poor stellar content of the central Milky Way.
Beers, Timothy C. +29 more
core +4 more sources
GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI
The observations from the Dark Energy Spectroscopic Instrument (DESI) will significantly increase the numbers of known extremely metal-poor stars by a factor of ∼10, improving the sample statistics to study the early chemical evolution of the Milky Way ...
Carlos Allende Prieto +50 more
doaj +1 more source
SEARCHING FOR DUST AROUND HYPER METAL POOR STARS [PDF]
Accepted for publication in ...
Venn, Kim A. +5 more
openaire +4 more sources
High-Resolution Spectroscopic Study of Extremely Metal-Poor Star Candidates from the SkyMapper Survey [PDF]
The SkyMapper Southern Sky Survey is carrying out a search for the most metal-poor stars in the Galaxy. It identifies candidates by way of its unique filter set that allows for estimation of stellar atmospheric parameters.
Asplund, Martin +15 more
core +2 more sources
Pulsating Blue Metal-poor Stars
The blue metal-poor (BMP) star CS 22966-043 is an SX Phoenicis star and the primary of a spectroscopic binary with a provisional orbital period of ~430 days. Radial velocity and UBV photometric observations of this star made in 1998 require downward revision of the orbital period to 319 days. The BMP star CS 29499-057 also appears to be an SX Phoenicis
George W. Preston, Arlo U. Landolt
openaire +1 more source
Inefficient star formation in extremely metal poor galaxies [PDF]
Author's version (10 pages, 4 figures).
Shi, Yong +7 more
openaire +4 more sources

