Results 21 to 30 of about 11,182,421 (303)

The Transition from Population III to Population II Stars [PDF]

open access: yesThe Astrophysical Journal, 2004
4 pages, 2 figures.
Fang, Taotao, Cen, Renyue
openaire   +2 more sources

Theoretical results of one class of multiderivative methods through order stars [PDF]

open access: yes, 2011
Order stars are applied to Brown (K,L) methods. They are displayed pictorially for a selection of methods and are used to provide succinct proofs of existing results.
Meneguette, Messias   +6 more
core   +3 more sources

Modelling and observations of molecules in discs around young stars [PDF]

open access: yes, 2013
This thesis contains a study of molecules within circumstellar discs around young stars. Firstly, the chemistry of a disc around a young, Class 0 protostar is modelled.
Ilee, John David
core   +5 more sources

Populations of rotating stars [PDF]

open access: yesAstronomy & Astrophysics, 2013
Accepted for publication in A&A, language ...
Granada   +7 more
openaire   +2 more sources

Deficiency of Metals in Population II Stars [PDF]

open access: yesNature, 1963
IN a recent communication under this title Bashkin1 has attempted to explain the deficiency of heavy elements in Population II halo stars by arguing that a separation between neutral atoms and ions is possible through electromagnetic means and that, since the ionization potentials of the metals are in general low, they will be confined to the disk ...
GEORGE WALLERSTEIN, E. MARGARET BURBIDGE
openaire   +3 more sources

Lithium In Population II Stars [PDF]

open access: yesHighlights of Astronomy, 1995
AbstractSince the work of Spite & Spite (1982), halo main sequence turn-off stars have usually been considered a site where Li synthesized in the Big-Bang is wholly preserved and uncontaminated by other Li sources. However, the interpretation of halo dwarf Li abundances has become more complex as new samples of halo star Li I observations have ...
openaire   +1 more source

Footprints of population III stars in the gravitational-wave background

open access: yes, 2021
International audienceWe investigate detection prospects of the gravitational-wave background (GWB) that originates from the merging of compact objects formed by the collapse of population III stars.
Sakellariadou, Mairi; id_orcid   +4 more
core   +1 more source

Spectroscopic survey of Kepler stars – II. FIES/NOT observations of A- and F-type stars [PDF]

open access: yes, 2017
We have analysed high-resolution spectra of 28 A and 22 F stars in the Kepler field, observed using the Fibre-Fed Échelle Spectrograph at the Nordic Optical Telescope. We provide spectral types, atmospheric parameters and chemical abundances for 50 stars.
S. J. Murphy   +22 more
core   +1 more source

Unique Chemical Composition of the Very Metal-poor Star LAMOST J1645+4357

open access: yesThe Astrophysical Journal, 2023
We report on the chemical composition of the very metal-poor (VMP; [Fe/H] = −2.9) star LAMOST J1645+4357, which was identified as a red giant having peculiar abundance ratios by Li et al. The standard abundance analysis is carried out for this object and
Wako Aoki   +5 more
doaj   +1 more source

Cosmic reionization by stellar sources: Population II stars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2003
We study the reionisation of the Universe by stellar sources using a numerical approach that combines fast 3D radiative transfer calculations with high resolution hydrodynamical simulations. Ionising fluxes for the sources are derived from intrinsic star formation rates computed in the underlying hydrodynamical simulations.
Sokasian, Aaron   +3 more
openaire   +5 more sources

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