The DOI matches its Crossref record.
Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster
Open accessAbstract
The isothermal gravitational collapse and fragmentation of a region within a molecular cloud and the subsequent formation of a protostellar cluster are investigated numerically. The clump mass spectrum that forms during the fragmentation phase can be well approximated by a power-law distribution dN / dM ∝ M −1.5 . In contrast, the mass spectrum of protostellar cores that form in the centers of Jeans-unstable clumps and that evolve through accretion and N -body interactions is described by a lognormal distribution with a width that is in excellent agreement with observations of multiple stellar systems.
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
Cited by
Star Formation in the Milky Way and Nearby Galaxies
Kennicutt, R. C., & Evans, N. J. (2012) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125610 · Cited by 2,902
“Simulations of unstable large clumps in fact tend to fragment so strongly as the mean density increases that they overproduce brown dwarfs, but no massive stars (e.g., Klessen et al. 1998; Martel et al. 2006).”
BackgroundControl of star formation by supersonic turbulence
Mac Low, M.-M., & Klessen, R. S. (2004) · Reviews of Modern Physics · doi:10.1103/revmodphys.76.125 · Cited by 1,761
Self-citationThe formation of a bound star cluster: from the Orion nebula cluster to the Pleiades
Kroupa, P., Aarseth, S., & Hurley, J. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04050.x · Cited by 458
Bate, M. R. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.14106.x · Cited by 440
Self-citationGravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
Klessen, R. S., Heitsch, F., & Mac Low, M. (2000) · The Astrophysical Journal · doi:10.1086/308891 · Cited by 419
Self-citation
Metadata
- Authors
- Klessen, R. S., Burkert, A., & Bate, M. R.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1998-07-10
- Volume
- 501
- Issue
- 2
- Pages
- L205-L208
- ISSN
- 0004-637X (ISSN-L)
- OpenAlex
- W2004460878
- Cited by
- 160
- References
- 0
- FWCI
- 9.61
- 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: Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster. https://app.cochat.ai/papers/10.1086/311471
- The paper
- Klessen, R. S., Burkert, A., & Bate, M. R. (1998). Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster. The Astrophysical Journal. https://doi.org/10.1086/311471
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.