- RESEARCH BRIEFINGS
Deep imaging of ionized gas in the Helix Nebula uncovers many curved shock waves around a dying Sun-like star. These ‘bow shocks’ are produced when ejected shells of stellar material break up and race outwards. Their changing shapes imply that the shell fragments are being stripped, shredded and mixed into interstellar gas over roughly 10,000 years.
This is a summary of: van Dokkum, P. et al. Numerous bow shocks in the outer Helix Nebula. Nature 656, 334–337 (2026).
doi: https://doi.org/10.1038/d41586-026-02159-3
‘Expert opinion’ is published under a CC BY 4.0 licence and Figure 1 is published under a CC BY-NC-ND 4.0 licence.
References
Kwok, S., Purton, C. R. & FitzGerald, P. M. Astrophys. J. 219, L125–L127 (1978).
Article Google Scholar
Karakas, A. I. & Lattanzio, J. C. Publ. Astron. Soc. Aust. 31, e030 (2014).
Article Google Scholar
O’Dell, C. R., McCullough, P. R. & Meixner, M. Astron. J. 128, 2339–2356 (2004).
Article Google Scholar
Chen, S. et al. Publ. Astron. Soc. Pac. 137, 084103 (2025).
Article Google Scholar
Klein, R. I., McKee, C. F. & Colella, P. Astrophys. J. 420, 213–236 (1994).
Article Google Scholar
Download references
Related Articles
-
Read the paper: Numerous bow shocks in the outer Helix Nebula
-
Dying star reveals its inner structure
-
Ultra-bright supernova wobbles like a spinning top
Subjects
Latest on:
- Astronomy and astrophysics
-
Evidence for the first globular cluster stellar stream beyond the Milky Way
Article
-
A gas-enshrouded and gas-reddened black hole at cosmic dawn
Article
-
Numerous bow shocks in the outer Helix Nebula
Article