Binary and multiple star systems result from the fragmentation of dense material in young molecular clouds. Observations reveal that this can occur on small scales, supporting a previous model of star formation. See Letter p.483
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
Rent or buy this article
Prices vary by article type
from$1.95
to$39.95
Prices may be subject to local taxes which are calculated during checkout
Notes
References
Raghavan, D. et al. Astrophys. J. Suppl. 190, 1–42 (2010).
Tobin, J. J. et al. Nature 538, 483–486 (2016).
Evans, N. J. II et al. Astrophys. J. Suppl. 181, 321–350 (2009).
Mathieu, R. D. Annu. Rev. Astron. Astrophys. 32, 465–530 (1994).
Duchêne, G. & Kraus, A. Annu. Rev. Astron. Astrophys. 51, 269–310 (2013).
Reipurth, B. et al. in Protostars and Planets Vol. VI (eds Beuther, H. et al.) 267–290 (Univ. Arizona Press, 2014).
Pineda, J. E. Nature 518, 213–215 (2015).
Toomre, A. Astrophys. J. 139, 1217–1238 (1964).
Author information
Authors and Affiliations
Corresponding author
Related links
Related links
Related links in Nature Research
Astrophysics: Violent emissions of newborn stars
Rights and permissions
About this article
Cite this article
Plunkett, A. Birth of stellar siblings. Nature 538, 466–467 (2016). https://doi.org/10.1038/538466a
Published:
Issue Date:
DOI: https://doi.org/10.1038/538466a