Stress drives gas into a black hole
Kartik Sheth () and
Peter J. Teuben ()
Additional contact information
Kartik Sheth: University of Maryland
Peter J. Teuben: University of Maryland
Nature, 1999, vol. 397, issue 6717, 298-299
Abstract:
New measurements of polarized radio emission from a barred spiral galaxy have allowed researchers to determine the galactic magnetic field, and to link it to interstellar gas flow in the bar region. Their results suggest that magnetic stress may be an efficient way of fuelling the supermassive black hole thought to exist in the active galactic nucleus of many galaxies.
Date: 1999
References: Add references at CitEc
Citations:
Downloads: (external link)
https://www.nature.com/articles/16802 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:397:y:1999:i:6717:d:10.1038_16802
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/16802
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 ().