Weighing in on neutron stars
M. Coleman Miller
Additional contact information
M. Coleman Miller: University of Maryland, and the Joint Space Science Institute, College Park, Maryland 20742–2421, USA. miller@astro.umd.edu
Nature, 2010, vol. 467, issue 7319, 1057-1058
Abstract:
The more massive a neutron star is, the greater the constraints it places on the nature of the matter at its core. The discovery of a new mass record holder has strengthened those constraints considerably. See Letter p.1081
Date: 2010
References: Add references at CitEc
Citations:
Downloads: (external link)
https://www.nature.com/articles/4671057a Abstract (text/html)
Access to the full text of the articles in this series is restricted.
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:467:y:2010:i:7319:d:10.1038_4671057a
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/4671057a
Access Statistics for this article
Nature is currently edited by Magdalena Skipper
More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().