Deep-imaging observations of the Andromeda galaxy and its surroundings have revealed a wide but thin planar structure of satellite galaxies that all orbit their host in the same rotational direction. See Letter p.62
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 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
Change history
16 January 2013
A Correction to this paper has been published: https://doi.org/10.1038/493315a
References
Ibata, R. A. et al. Nature 493, 62–65 (2013).
Lynden-Bell, D. Mon. Not. R. Astron. Soc. 174, 695–710 (1976).
Pawlowski, M. S., Pflamm-Altenburg, J. & Kroupa, P. Mon. Not. R. Astron. Soc. 423, 1109–1126 (2012).
Karachentsev, I. D. et al. Astron. Astrophys. 385, 21–31 (2002).
Chiboucas, K., Karachentsev, I. D. & Tully, R. B. Astron. J. 137, 3009–3037 (2009).
Tully, R. B. et al. Astrophys. J. 676, 184–205 (2008).
Klypin, A., Kravtsov, A. V., Valenzuela, O. & Prada, F. Astrophys. J. 522, 82–92 (1999).
Moore, B. et al. Astrophys. J. 524, L19–L22 (1999).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Tully, R. Andromeda's extended disk of dwarfs. Nature 493, 31–32 (2013). https://doi.org/10.1038/493031a
Published:
Issue Date:
DOI: https://doi.org/10.1038/493031a
This article is cited by
-
Correction
Nature (2013)