Results 31 to 40 of about 197,137 (264)

On the Mass of Population III Stars [PDF]

open access: yesThe Astrophysical Journal, 1999
Performing 1D hydrodynamical calculations coupled with non-equilibrium processes for H2 formation, we pursue the thermal and dynamical evolution of filamentary primordial clouds and attempt to make an estimate on the mass of population III stars. It is found that, almost independent of initial conditions, a filamentary cloud continues to collapse ...
Nakamura, Fumitaka, Umemura, Masayuki
openaire   +2 more sources

GW231123 Formation from Population III Stars: Isolated Binary Evolution [PDF]

open access: yesAstrophysical Journal
GW231123 is a merger of two black holes (BHs) with estimated masses exceeding 100 M⊙, making them the most massive BHs discovered to date via gravitational-wave (GW) observations.
A. Tanikawa   +4 more
semanticscholar   +1 more source

THE MOST IRON-DEFICIENT STARS AS THE POLLUTED POPULATION III STARS [PDF]

open access: yesThe Astrophysical Journal, 2015
Accepted for publication in ApJ ...
Yutaka Komiya   +2 more
openaire   +2 more sources

Explaining the high nitrogen abundances observed in high-z galaxies via population III stars of a few thousand solar masses [PDF]

open access: yesAstronomy & Astrophysics
Efforts to understand the origin and growth of massive black holes observed in the early Universe have spurred a strong interest in the evolution and fate of rapidly-accreting primordial (metal-free) stars.
D. Nandal   +5 more
semanticscholar   +1 more source

Predicting the observability of population III stars with ELT-HARMONI via the helium 1640 Å emission line [PDF]

open access: yes, 2021
Population III (Pop. III) stars, as of yet, have not been detected, however as we move into the era of extremely large telescopes this is likely to change. One likely tracer for Pop.
Kearn Grisdale   +7 more
semanticscholar   +1 more source

POPULATION III STARS AROUND THE MILKY WAY [PDF]

open access: yesThe Astrophysical Journal, 2016
ABSTRACT We explore the possibility of observing Population III (Pop III) stars, born of primordial gas. Pop III stars with masses below 0.8 M ⊙ should survive to date though are not yet observed, but the existence of stars with low metallicity as
Yutaka Komiya   +2 more
openaire   +2 more sources

JADES. Possible Population III signatures at z=10.6 in the halo of GN-z11 [PDF]

open access: yesAstronomy & Astrophysics, 2023
Finding the first generation of stars formed out of pristine gas in the early Universe, known as Population III (PopIII) stars, is one of the most important goals of modern astrophysics.
R. Maiolino   +33 more
semanticscholar   +1 more source

Gamma-Ray Bursts and Population III Stars [PDF]

open access: yesSpace Science Reviews, 2016
27 pages, 5 figures, an output from ISSI-BJ Workshop on Gamma-Ray Bursts: a tool to explore the young Universe, accepted for publication in Space Science ...
Toma, Kenji   +2 more
openaire   +2 more sources

Contribution of population III stars to merging binary black holes [PDF]

open access: yesReviews of Modern Plasma Physics
A large number of mergers of binary black holes (BHs) have been discovered by gravitational wave observations since the first detection of gravitational waves 2015.
A. Tanikawa
semanticscholar   +1 more source

MAGNETIC FIELDS IN POPULATION III STAR FORMATION [PDF]

open access: yesThe Astrophysical Journal, 2012
We study the buildup of magnetic fields during the formation of Population III star-forming regions, by conducting cosmological simulations from realistic initial conditions and varying the Jeans resolution. To investigate this in detail, we start simulations from identical initial conditions, mandating 16, 32 and 64 zones per Jeans length, and studied
Turk, Matthew J.   +3 more
openaire   +3 more sources

Home - About - Disclaimer - Privacy