The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
STAR FORMATION RELATIONS IN NEARBY MOLECULAR CLOUDS
Open accessAbstract
We test some ideas for star formation relations against data on local molecular clouds. On a cloud by cloud basis, the relation between the surface density of star formation rate and surface density of gas divided by a free-fall time, calculated from the mean cloud density, shows no significant correlation. If a crossing time is substituted for the free-fall time, there is even less correlation. Within a cloud, the star formation rate volume and surface densities increase rapidly with the corresponding gas densities, faster than predicted by models using the free-fall time defined from the local density. A model in which the star formation rate depends linearly on the mass of gas above a visual extinction of 8 mag describes the data on these clouds, with very low dispersion. The data on regions of very massive star formation, with improved star formation rates based on free–free emission from ionized gas, also agree with this linear relation.
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 10×
“This Σ(SFR) is much lower than in the inner parts of the Galaxy or in many regions studied in other galaxies, but it is close to Electronic address: nje@astro.as.utexas.edu the average value over the inner 13.5 kpc of the Galaxy (Kennicutt and Evans 2012).”
BackgroundInfluentialSelf-citationTHE STAR FORMATION EFFICIENCY IN NEARBY GALAXIES: MEASURING WHERE GAS FORMS STARS EFFECTIVELY
Leroy, A. K., Walter, F., Brinks, E., Bigiel, F., de Blok, W. J. G., Madore, B., & Thornley, M. D. (2008) · The Astronomical Journal · doi:10.1088/0004-6256/136/6/2782 · Cited by 1,919
Variations in the Galactic star formation rate and density thresholds for star formation
Longmore, S. N., Bally, J., Testi, L., Purcell, C. R., Walsh, A. J., Bressert, E., Pestalozzi, M., Molinari, S., Ott, J., Cortese, L., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts376 · Cited by 357
Cited by
Könyves, V., André, P., Men’shchikov, A., Palmeirim, P., Arzoumanian, D., Schneider, N., Roy, A., Didelon, P., Maury, A., Shimajiri, Y., et al. (2015) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201525861 · Cited by 486
PHANGS–ALMA: Arcsecond CO(2–1) Imaging of Nearby Star-forming Galaxies
Leroy, A. K., Schinnerer, E., Hughes, A., Rosolowsky, E., Pety, J., Schruba, A., Usero, A., Blanc, G. A., Chevance, M., Emsellem, E., et al. (2021) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ac17f3 · Cited by 391
Krumholz, M. R. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.001 · Cited by 321
A unified model for galactic discs: star formation, turbulence driving, and mass transport
Krumholz, M. R., Burkhart, B., Forbes, J. C., & Crocker, R. M. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty852 · Cited by 319
Dark matter cores all the way down
Read, J. I., Agertz, O., & Collins, M. L. M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw713 · Cited by 318
Metadata
- Authors
- Evans, N. J., Heiderman, A., & Vutisalchavakul, N.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2014-02-04
- Volume
- 782
- Issue
- 2
- Pages
- 114
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2037247549
- Cited by
- 241
- References
- 3
- FWCI
- 12.91
- 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: STAR FORMATION RELATIONS IN NEARBY MOLECULAR CLOUDS. https://app.cochat.ai/papers/10.1088/0004-637x/782/2/114
- The paper
- Evans, N. J., Heiderman, A., & Vutisalchavakul, N. (2014). STAR FORMATION RELATIONS IN NEARBY MOLECULAR CLOUDS. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/782/2/114
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.