The DOI matches its Crossref record; 51 of the 51 references it cites were found in a registry or an index.
Protostellar Feedback Halts the Growth of the First Stars in the Universe
Open accessAbstract
Simulations suggest that most of the first stars in the universe might have been less massive than previously thought.
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Citations
Cites
Galactic Stellar and Substellar Initial Mass Function
Chabrier, G. (2003) · Publications of the Astronomical Society of the Pacific · doi:10.1086/376392 · Cited by 9,071
Galactic Stellar and Substellar Initial Mass FunctionPreprint
Chabrier, G. (2003) · Cited by 4,970
Astrophysics of Gaseous Nebulae and Active Galactic Nuclei
Osterbrock, D. E., & Michael Shull, J. (1989) · Physics Today · doi:10.1063/1.2811187 · Cited by 3,699
Astrophysics of gaseous nebulae and active galactic nuclei
(1989) · Choice Reviews Online · doi:10.5860/choice.26-6270 · Cited by 2,052
The Nucleosynthetic Signature of Population III
Heger, A., & Woosley, S. E. (2002) · The Astrophysical Journal · doi:10.1086/338487 · Cited by 1,669
Black Holes in Binary Systems: Observational Appearances
Shakura, N. I., & Sunyaev, R. A. (1973) · X- and Gamma-Ray Astronomy · doi:10.1007/978-94-010-2585-0_13 · Cited by 1,503
The Formation of the First Star in the Universe
Abel, T., Bryan, G. L., & Norman, M. L. (2002) · Science · doi:10.1126/science.1063991 · Cited by 1,448
Photodissociation regions. I - Basic model. II - A model for the Orion photodissociation region
Tielens, A. G. G. M., & Hollenbach, D. (1985) · The Astrophysical Journal · doi:10.1086/163111 · Cited by 1,256
On the properties of massive Population III stars and metal-free stellar populations
Schaerer, D. (2002) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20011619 · Cited by 878
Molecule formation and infrared emission in fast interstellar shocks. I Physical processes
Hollenbach, D., & McKee, C. F. (1979) · The Astrophysical Journal Supplement Series · doi:10.1086/190631 · Cited by 771
Cited by
The Assembly of the First Massive Black Holes
Inayoshi, K., Visbal, E., & Haiman, Z. (2020) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-120419-014455 · Cited by 665
Near-Field Cosmology with Extremely Metal-Poor Stars
Frebel, A., & Norris, J. E. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122423 · Cited by 533
FORMATION OF PRIMORDIAL SUPERMASSIVE STARS BY RAPID MASS ACCRETION
Hosokawa, T., Yorke, H. W., Inayoshi, K., Omukai, K., & Yoshida, N. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/778/2/178 · Cited by 295
Self-citationBuilding 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
Metadata
- Authors
- Hosokawa, T., Omukai, K., Yoshida, N., & Yorke, H. W.
- Venue
- Science
- Published
- 2011-12-02
- Volume
- 334
- Issue
- 6060
- Pages
- 1250-1253
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2073753053
- Cited by
- 386
- References
- 51
- FWCI
- 22.12
- Type
- journal article
- Language
- en
- Open access
- green
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- CoChat. (2026). Citation check: Protostellar Feedback Halts the Growth of the First Stars in the Universe. https://app.cochat.ai/papers/10.1126/science.1207433
- The paper
- Hosokawa, T., Omukai, K., Yoshida, N., & Yorke, H. W. (2011). Protostellar Feedback Halts the Growth of the First Stars in the Universe. Science. https://doi.org/10.1126/science.1207433
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.
