EconPapers    
Economics at your fingertips  
 

How pulsars get their spins

Adam Burrows ()
Additional contact information
Adam Burrows: University of Arizona

Nature, 1998, vol. 393, issue 6681, 121-122

Abstract: A supernova explosion announces the spectacular death of a massive star. The remnant is usually a neutron star, tiny and dense, and often spinning rapidly and travelling at high speed through the Galaxy. A provocative new thesis forms a bridge between the physics of supernovae and the spin and velocity of neutron stars.

Date: 1998
References: Add references at CitEc
Citations:

Downloads: (external link)
https://www.nature.com/articles/30108 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:393:y:1998:i:6681:d:10.1038_30108

Ordering information: This journal article can be ordered from
https://www.nature.com/

DOI: 10.1038/30108

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 ().

 
Page updated 2025-03-19
Handle: RePEc:nat:nature:v:393:y:1998:i:6681:d:10.1038_30108