File:Neutronstar MassRadius Thomas2013 epjconf-hias2013-03004 fig2.svg
Jump to navigation
Jump to search
Original file (SVG file, nominally 1,410 × 1,700 pixels, file size: 65 KB)
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 |
Licensing
This file is licensed under the Creative Commons Attribution 2.5 Generic license.
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 17:46, 7 May 2019 | | 1,410 × 1,700 (65 KB) | wikimediacommons>Geek3 | User created page with UploadWizard |
File usage
There are no pages that use this file.
