Magnetic bond

Christopher M. Johns-Krull
Additional contact information
Christopher M. Johns-Krull: Rice University, 6100 Main Street, Houston, Texas 77005, USA. cmj@rice.edu

Nature, 2009, vol. 457, issue 7226, 158-159

Abstract: How low-mass stars produce their ubiquitous magnetic fields has long puzzled astronomers. Models of how Earth accomplishes this task could hold the key to understanding the phenomenon on such stars.

Date: 2009
References: Add references at CitEc
Citations:

Downloads: (external link)
https://www.nature.com/articles/457158a 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:457:y:2009:i:7226:d:10.1038_457158a

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

DOI: 10.1038/457158a

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 ().