The winds from growing supermassive black holes appear to be located tens of parsecs from the centres of their host galaxies. This location fits with the idea that these outflows influence the progression of star formation.
This is a preview of subscription content, access via your institution
Access options
Access Nature and 54 other Nature Portfolio journals
Get Nature+, our best-value online-access subscription
$29.99 / 30 days
cancel any time
Subscribe to this journal
Receive 12 digital issues and online access to articles
$119.00 per year
only $9.92 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Murray, N., Chiang, J., Grossman, S. A. & Voit, G. M. Astrophys. J. 451, 498–509 (1995).
He, Z. et al. Nat. Astron. https://doi.org/10.1038/s41550-018-0669-8 (2019).
Ferrarrese, L. & Merritt, D. Astrophys. J. 539, L9–L12 (2000).
Hopkins, P. F. et al. Astrophys. J. Suppl. Ser. 163, 1–49 (2006).
Leighly, K. M. et al. Astrophys. J. 788, 123 (2014).
Fabian, A. C. Ann. Rev. Astron. Astrophys. 50, 455–489 (2012).
Hewett, P. C. & Foltz, C. B. Astron. J. 125, 1784–1794 (2003).
de Kool, M. et al. Astrophys. J. 548, 609–623 (2001).
Filik Ak, N. et al. Astrophys. J. 777, 168 (2013).
Leighly, K. M., Terndrup, D. M., Gallagher, S. C., Richards, G. T. & Dietrich, M. Astrophys. J. 866, 7 (2018).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Gallagher, S.C. Where is the wind?. Nat Astron 3, 202–203 (2019). https://doi.org/10.1038/s41550-019-0702-6
Published:
Issue Date:
DOI: https://doi.org/10.1038/s41550-019-0702-6
