Student or educator? Sign up with your school email and get 6 months of Pro free.
Cited by 348

The DOI matches its Crossref record.

Intense star formation within resolved compact regions in a galaxy at z = 2.3

Open access
Swinbank, A. M., Smail, I., Longmore, S., Harris, A. I., Baker, A. J., De Breuck, C., Richard, J., Edge, A. C., Ivison, R. J., Blundell, R., Coppin, K. E. K., Cox, P., Gurwell, M., Hainline, L. J., Krips, M., Lundgren, A., Neri, R., Siana, B., Siringo, G., Stark, D. P., Wilner, D., Younger, J. D.·2010·Nature

Abstract

Massive galaxies in the early Universe have been shown to be forming stars at surprisingly high rates. Prominent examples are dust-obscured galaxies which are luminous when observed at sub-millimetre wavelengths and which may be forming stars at a rate of 1,000 solar masses (M⊙) per year. These intense bursts of star formation are believed to be driven by mergers between gas-rich galaxies. Probing the properties of individual star-forming regions within these galaxies, however, is beyond the spatial resolution and sensitivity of even the largest telescopes at present. Here we report observations of the sub-millimetre galaxy SMMJ2135-0102 at redshift z = 2.3259, which has been gravitationally magnified by a factor of 32 by a massive foreground galaxy cluster lens. This magnification, when combined with high-resolution sub-millimetre imaging, resolves the star-forming regions at a linear scale of only 100 parsecs. We find that the luminosity densities of these star-forming regions are comparable to the dense cores of giant molecular clouds in the local Universe, but they are about a hundred times larger and 107 times more luminous. Although vigorously star-forming, the underlying physics of the star-formation processes at z ≈ 2 appears to be similar to that seen in local galaxies, although the energetics are unlike anything found in the present-day Universe.

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.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1038/nature08880

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.

A few free checks a day · papers already verified open instantly · results are public

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

See all 348

Metadata

Authors
Swinbank, A. M., Smail, I., Longmore, S., Harris, A. I., Baker, A. J., De Breuck, C., Richard, J., Edge, A. C., Ivison, R. J., Blundell, R., Coppin, K. E. K., Cox, P., Gurwell, M., Hainline, L. J., Krips, M., Lundgren, A., Neri, R., Siana, B., Siringo, G., Stark, D. P., Wilner, D., & Younger, J. D.
Venue
Nature
Published
2010-03-21
Volume
464
Issue
7289
Pages
733-736
ISSN
  • 0028-0836 (ISSN-L)
  • 1476-4687
OpenAlex
W2031076586
Cited by
348
References
0
FWCI
22.25
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: Intense star formation within resolved compact regions in a galaxy at z = 2.3. https://app.cochat.ai/papers/10.1038/nature08880
The paper
Swinbank, A. M., Smail, I., Longmore, S., Harris, A. I., Baker, A. J., De Breuck, C., Richard, J., Edge, A. C., Ivison, R. J., Blundell, R., Coppin, K. E. K., Cox, P., Gurwell, M., Hainline, L. J., Krips, M., Lundgren, A., Neri, R., Siana, B., Siringo, G., . . . Younger, J. D. (2010). Intense star formation within resolved compact regions in a galaxy at z = 2.3. Nature. https://doi.org/10.1038/nature08880

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.