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Star formation

Three's a crowd

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An Erratum to this article was published on 15 June 2000

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Figure 1: Star rating.
Figure 2: Millimetre-wave image of a cluster of four young protostars in a nearby star-forming region, NGC1333.

Notes

  1. *The Formation of Binary Stars International Astronomical Union Symposium 200. Potsdam, Germany, 10–15 April 2000.

References

  1. Shu, F. H., Adams, F. C. & Lizano, S. Annu. Rev. Astron. Astrophys. 25, 23–72 (1987).

    Article  ADS  CAS  Google Scholar 

  2. Mathieu, R. D. Annu. Rev. Astron. Astrophys. 32, 465–530 (1994).

    Article  ADS  Google Scholar 

  3. Ghez, A. M., McCarthy, D. W., Patience, J. L. & Beck, T. L. Astrophys. J. 481, 378–385 (1997).

    Article  ADS  Google Scholar 

  4. Rodriguez, L. F. et al. Nature 395, 355–356 (1998).

    Article  ADS  CAS  Google Scholar 

  5. Clarke, C. J. & Pringle, J. E. Mon. Not. R. Astron. Soc. 249, 584–587 (1991).

    Article  ADS  Google Scholar 

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Correspondence to Alan P. Boss.

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Boss, A. Three's a crowd. Nature 405, 405–407 (2000). https://doi.org/10.1038/35013174

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