The DOI matches its Crossref record; 45 of the 45 references it cites were found in a registry or an index.
Population III stars: hidden or disappeared?
Open accessAbstract
A Population III/Population II transition from massive to normal stars is predicted to occur when the metallicity of the star-forming gas crosses the critical range Zcr= 10−5±1 Z⊙. To investigate the cosmic implications of such a process, we use numerical simulations which follow the evolution, metal enrichment and energy deposition of both Population II and Population III stars. We find that: (i) due to inefficient heavy element transport by outflows and slow ‘genetic’ transmission during hierarchical growth, large fluctuations around the average metallicity arise; as a result, Population III star formation continues down to z= 2.5, but at a low peak rate of 10−5 M⊙ yr−1 Mpc−3 occurring at z≈ 6 (about 10−4 of the Population II one); and (ii) Population III star formation proceeds in an ‘inside–out’ mode in which formation sites are progressively confined to the periphery of collapsed structures, where the low gas density and correspondingly long free-fall time-scales result in a very inefficient astration. These conclusions strongly encourage deep searches for pristine star formation sites at moderate (2 < z < 5) redshifts where metal-free stars are likely to be hidden.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
Spergel, D. N., Bean, R., Dore, O., Nolta, M. R., Bennett, C. L., Dunkley, J., Hinshaw, G., Jarosik, N., Komatsu, E., Page, L., et al. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/513700 · Cited by 6,778
The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
Woosley, S. E., & Weaver, T. A. (1995) · The Astrophysical Journal Supplement Series · doi:10.1086/192237 · Cited by 3,761
Cooling functions for low-density astrophysical plasmas
Sutherland, R. S., & Dopita, M. A. (1993) · The Astrophysical Journal Supplement Series · doi:10.1086/191823 · Cited by 2,434
The Nucleosynthetic Signature of Population III
Heger, A., & Woosley, S. E. (2002) · The Astrophysical Journal · doi:10.1086/338487 · Cited by 1,669
Radiative Transfer in a Clumpy Universe. II. The Ultraviolet Extragalactic Background
Haardt, F., & Madau, P. (1996) · The Astrophysical Journal · doi:10.1086/177035 · Cited by 1,570
Shapley, A. E., Steidel, C. C., Pettini, M., & Adelberger, K. L. (2003) · The Astrophysical Journal · doi:10.1086/373922 · Cited by 1,407
The Discovery and Analysis of Very Metal-Poor Stars in the Galaxy
Beers, T. C., & Christlieb, N. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.134057 · Cited by 1,223
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Cayrel, R., Depagne, E., Spite, M., Hill, V., Spite, F., François, P., Plez, B., Beers, T., Primas, F., Andersen, J., et al. (2004) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20034074 · Cited by 1,154
Simulations of Early Structure Formation: Primordial Gas Clouds
Yoshida, N., Abel, T., Hernquist, L., & Sugiyama, N. (2003) · The Astrophysical Journal · doi:10.1086/375810 · Cited by 574
Cited by
Bromm, V., & Yoshida, N. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102608 · Cited by 512
THE BIRTH OF A GALAXY: PRIMORDIAL METAL ENRICHMENT AND STELLAR POPULATIONS
Wise, J. H., Turk, M. J., Norman, M. L., & Abel, T. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/745/1/50 · Cited by 462
FORMATION OF THE FIRST NUCLEAR CLUSTERS AND MASSIVE BLACK HOLES AT HIGH REDSHIFT
Devecchi, B., & Volonteri, M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/694/1/302 · Cited by 310
Building up the Population III initial mass function from cosmological initial conditions
Stacy, A., Bromm, V., & Lee, A. T. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1728 · Cited by 257
The oldest and most metal-poor stars in the APOSTLE Local Group simulations
Starkenburg, E., Oman, K. A., Navarro, J. F., Crain, R. A., Fattahi, A., Frenk, C. S., Sawala, T., & Schaye, J. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2873 · Cited by 85
Metadata
- Authors
- Tornatore, L., Ferrara, A., & Schneider, R.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2007-11-08
- Volume
- 382
- Issue
- 3
- Pages
- 945-950
- ISSN
- 0035-8711 (ISSN-L)
- OpenAlex
- W1786516248
- Cited by
- 253
- References
- 45
- FWCI
- 9.66
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Population III stars: hidden or disappeared? https://app.cochat.ai/papers/10.1111/j.1365-2966.2007.12215.x
- The paper
- Tornatore, L., Ferrara, A., & Schneider, R. (2007). Population III stars: hidden or disappeared? Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2007.12215.x
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.