Student or educator? Sign up with your school email and get 6 months of Pro free.
Cited by 355

The DOI matches its Crossref record; 20 of the 20 references it cites were found in a registry or an index.

Connecting Dense Gas Tracers of Star Formation in our Galaxy to High- z Star Formation

Open access
Wu, Jingwen, Evans II, Neal J., Gao, Yu, Solomon, Philip M., Shirley, Yancy L., Vanden Bout, Paul A.·2005·The Astrophysical Journal

Abstract

Observations have revealed prodigious amounts of star formation in starburst galaxies as traced by dust and molecular emission, even at large redshifts. Recent work shows that for both nearby spiral galaxies and distant starbursts, the global star formation rate, as indicated by the infrared luminosity, has a tight and almost linear correlation with the amount of dense gas as traced by the luminosity of HCN. Our surveys of Galactic dense cores in HCN 1-0 emission show that this correlation continues to a much smaller scale, with nearly the same ratio of infrared luminosity to HCN luminosity found over 7-8 orders of magnitude in L IR , with a lower cutoff around 10 4.5 L ☉ of infrared luminosity. The linear correlation suggests that we may understand distant star formation in terms of the known properties of local star-forming regions. Both the correlation and the luminosity cutoff can be explained if the basic unit of star formation in galaxies is a dense core, similar to those studied in our Galaxy.

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 · 10.1086/499623

Cites

20 of 20 references verified0 citation errors · 0 not checkable

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

Cites

Show all 20 references

Cited by

See all 355

Metadata

Authors
Wu, J., Evans II, N. J., Gao, Y., Solomon, P. M., Shirley, Y. L., & Vanden Bout, P. A.
Venue
The Astrophysical Journal
Published
2005-12-06
Volume
635
Issue
2
Pages
L173-L176
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2137755072
Cited by
355
References
20
FWCI
8.78
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: Connecting Dense Gas Tracers of Star Formation in our Galaxy to High- z Star Formation. https://app.cochat.ai/papers/10.1086/499623
The paper
Wu, J., Evans II, N. J., Gao, Y., Solomon, P. M., Shirley, Y. L., & Vanden Bout, P. A. (2005). Connecting Dense Gas Tracers of Star Formation in our Galaxy to High- z Star Formation. The Astrophysical Journal. https://doi.org/10.1086/499623

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.