The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Turbulent molecular clouds
Open accessAbstract
Stars form within molecular clouds but our understanding of this fundamental process remains hampered by the complexity of the physics that drives their evolution. We review our observational and theoretical knowledge of molecular clouds trying to confront the two approaches wherever possible. After a broad presentation of the cold interstellar medium and molecular clouds, we emphasize the dynamical processes with special focus to turbulence and its impact on cloud evolution. We then review our knowledge of the velocity, density and magnetic fields. We end by openings towards new chemistry models and the links between molecular cloud structure and star-formation rates.
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
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 · cited 2×
“Direct comparisons with SFR inferred from observations (e.g. Heiderman et al. 2010, Kennicutt and Evans, 2012) have been performed but given the relatively large scatter of the data, it seems hard to draw firm conclusions.”
BackgroundMethodThe Three-Phase Interstellar Medium Revisited
Cox, D. P. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.43.072103.150615 · Cited by 417
Cited by
Molecular Clouds in the Milky Way
Heyer, M., & Dame, T. M. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122324 · Cited by 536
PHYSICAL PROPERTIES OF MOLECULAR CLOUDS FOR THE ENTIRE MILKY WAY DISK
Miville-Deschênes, M.-A., Murray, N., & Lee, E. J. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/834/1/57 · Cited by 396
Global hierarchical collapse in molecular clouds. Towards a comprehensive scenario
Vázquez-Semadeni, E., Palau, A., Ballesteros-Paredes, J., Gómez, G. C., & Zamora-Avilés, M. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2736 · Cited by 361
Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey
LiteBIRD Collaboration, Allys, E., Arnold, K., Aumont, J., Aurlien, R., Azzoni, S., Baccigalupi, C., Banday, A. J., Banerji, R., Barreiro, R. B., et al. (2023) · Progress of Theoretical and Experimental Physics · doi:10.1093/ptep/ptac150 · Cited by 348
Krumholz, M. R. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.001 · Cited by 321
Metadata
- Authors
- Hennebelle, P., & Falgarone, E.
- Venue
- The Astronomy and Astrophysics Review
- Published
- 2012-10
- Volume
- 20
- Issue
- 1
- ISSN
- 0935-4956 (ISSN-L)
- 1432-0754
- OpenAlex
- W2030648370
- Cited by
- 363
- References
- 2
- FWCI
- 12.23
- Type
- journal article
- Language
- en
- Open access
- green
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: Turbulent molecular clouds. https://app.cochat.ai/papers/10.1007/s00159-012-0055-y
- The paper
- Hennebelle, P., & Falgarone, E. (2012). Turbulent molecular clouds. The Astronomy and Astrophysics Review. https://doi.org/10.1007/s00159-012-0055-y
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.