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Cited by 373

The DOI matches its Crossref record.

On the Fragmentation of Gas Clouds Into Galaxies and Stars.

Hoyle, F.·1953·The Astrophysical Journal

Abstract

The present paper seeks to trace the steps whereby an extensive cloud of density 10 gm/cm3 evolves, first into galaxies and then into stars. The indication is that galaxies are likely to form, not as single objects, but in clusters. Stars apparently form at an early stage in the history of a galaxy. There would seem to be reason why the average mass of such stars should lie somewhat below the solar mass.

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Metadata

Authors
Hoyle, F.
Venue
The Astrophysical Journal
Published
1953-11
Volume
118
Pages
513
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1972072317
Cited by
373
References
0
FWCI
0.00
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: On the Fragmentation of Gas Clouds Into Galaxies and Stars. https://app.cochat.ai/papers/10.1086/145780
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Hoyle, F. (1953). On the Fragmentation of Gas Clouds Into Galaxies and Stars. The Astrophysical Journal. https://doi.org/10.1086/145780

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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.