File:Neutronstar MassRadius Thomas2013 epjconf-hias2013-03004 fig2.svg
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Summary
| Description |
English: Neutron star Gravitational Mass versus radius relationship for various scenarios described in the text. The black dots represent maximum mass stars and the coloured bars represent observed pulsar constraints. At low density the BPS [24] EoS is used. |
| Date | |
| Source |
(2013). "Equation of State of Dense Matter and Consequences for Neutron Stars". EPJ Web of Conferences 63: 03004. DOI:10.1051/epjconf/20136303004. ISSN 2100-014X. Figure 2 |
| Author | A. W. Thomas, D. L. Whittenbury, J. D. Carroll, K. Tsushima, and J. R. Stone |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 15:46, 7 May 2019 | | 1,410 × 1,700 (65 KB) | wikimediacommons>Geek3 | User created page with UploadWizard |
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