Astronomers have suspected for some time that magnetic fields are a key ingredient in the accretion of material that surrounds young stars. New observations have just begun to reveal these fields in action. See Letter p.597
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 SpringerLink
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Stephens, I. W. et al. Nature 514, 597–599 (2014).
Valenti, J. A., Basri, G. & Johns, C. M. Astron. J. 106, 2024–2050 (1993).
Gullbring, E., Hartmann, L., Briceno, C. & Calvet, N. Astrophys. J. 492, 323–341 (1998).
Balbus, S. A. & Hawley, J. F. Rev. Mod. Phys. 70, 1–53 (1998).
Lazarian, A. J. J. Quant. Spectrosc. Radiat. Transf. 106, 225–256 (2007).
Rao, R., Girart, J. M., Lai, S.-P. & Marrone, D. P. Astrophys. J. 780, L6 (2014).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Johns-Krull, C. Secret ingredient exposed. Nature 514, 571–572 (2014). https://doi.org/10.1038/nature13932
Published:
Issue Date:
DOI: https://doi.org/10.1038/nature13932