The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.
A high-resolution image of atomic hydrogen in the M81 group of galaxies
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Citations
Cites
Toomre, A., & Toomre, J. (1972) · The Astrophysical Journal · doi:10.1086/151823 · Cited by 2,555
Ultraluminous infrared galaxies and the origin of quasars
Sanders, D. B., Soifer, B. T., Elias, J. H., Madore, B. F., Matthews, K., Neugebauer, G., & Scoville, N. Z. (1988) · The Astrophysical Journal · doi:10.1086/165983 · Cited by 2,072
Fueling starburst galaxies with gas-rich mergers
Barnes, J. E., & Hernquist, L. E. (1991) · The Astrophysical Journal · doi:10.1086/185978 · Cited by 968
Freedman, W. L., Hughes, S. M. G., Madore, B. F., Mould, J. R., Lee, M. G., Stetson, P. B., Kennicutt, R. C., Turner, A. M. S., Ferrarese, L., Ford, H. C., et al. (1994) · The Astrophysical Journal · doi:10.1086/174172 · Cited by 564
On the Spiral Structure of Disk Galaxies. III. Comparison with Observations
Lin, C. C., Yuan, C., & Shu, F. H. (1969) · The Astrophysical Journal · doi:10.1086/149907 · Cited by 438
The nature of the nuclear sources in M82 and NGC 253
Rieke, G. H., Lebofsky, M. J., Thompson, R. I., Low, F. J., & Tokunaga, A. T. (1980) · The Astrophysical Journal · doi:10.1086/157954 · Cited by 413
Dark matter in spiral galaxies. II - Galaxies with H I rotation curves
Kent, S. M. (1987) · The Astronomical Journal · doi:10.1086/114366 · Cited by 302
Structure and Properties of Nearby Galaxies
(1978) · Springer eBooks · doi:10.1007/978-94-009-9818-6 · Cited by 149
Cited by
Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
Kormendy, J., & Kennicutt, R. C. (2004) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.134024 · Cited by 1,732
HI4PI: a full-sky H i survey based on EBHIS and GASS
HI4PI Collaboration:, Ben Bekhti, N., Flöer, L., Keller, R., Kerp, J., Lenz, D., Winkel, B., Bailin, J., Calabretta, M. R., Dedes, L., et al. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201629178 · Cited by 1,637
HIGH-RESOLUTION ROTATION CURVES AND GALAXY MASS MODELS FROM THINGS
de Blok, W. J. G., Walter, F., Brinks, E., Trachternach, C., Oh, S.-H., & Kennicutt, R. C. (2008) · The Astronomical Journal · doi:10.1088/0004-6256/136/6/2648 · Cited by 940
The effect of galaxy mass ratio on merger-driven starbursts
Cox, T. J., Jonsson, P., Somerville, R. S., Primack, J. R., & Dekel, A. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12730.x · Cited by 493
Cool outflows in galaxies and their implications
Veilleux, S., Maiolino, R., Bolatto, A. D., & Aalto, S. (2020) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-019-0121-9 · Cited by 466
Metadata
- Authors
- Yun, M. S., Ho, P. T. P., & Lo, K. Y.
- Venue
- Nature
- Published
- 1994-12
- Volume
- 372
- Issue
- 6506
- Pages
- 530-532
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2061252407
- Cited by
- 480
- References
- 8
- FWCI
- 5.41
- Type
- journal article
- Language
- en
- Open access
- closed
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.
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How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: A high-resolution image of atomic hydrogen in the M81 group of galaxies. https://app.cochat.ai/papers/10.1038/372530a0
- The paper
- Yun, M. S., Ho, P. T. P., & Lo, K. Y. (1994). A high-resolution image of atomic hydrogen in the M81 group of galaxies. Nature. https://doi.org/10.1038/372530a0
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.
