Published April 22, 2009 | Version Published
Journal Article Open

Astrophysical jets: observations, numerical simulations, and laboratory experiments

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Space Telescope Science Institute
  • 3. ROR icon University of Tsukuba
  • 4. ROR icon Imperial College London
  • 5. ROR icon Dublin Institute For Advanced Studies
  • 6. ROR icon University of Turin
  • 7. ROR icon University of Chicago
  • 8. ROR icon Rice University
  • 9. ROR icon University of Rochester
  • 10. ROR icon Atomic Weapons Establishment
  • 11. ROR icon Centre Lasers Intenses et Applications

Abstract

This paper provides summaries of ten talks on astrophysical jets given at the HEDP/HEDLA-08 International Conference in St. Louis. The talks are topically divided into the areas of observation, numerical modeling, and laboratory experiment. One essential feature of jets, namely, their filamentary (i.e., collimated) nature, can be reproduced in both numerical models and laboratory experiments. Another essential feature of jets, their scalability, is evident from the large number of astrophysical situations where jets occur. This scalability is the reason why laboratory experiments simulating jets are possible and why the same theoretical models can be used for both observed astrophysical jets and laboratory simulations.

Additional Information

© 2009 American Institute of Physics. Received 13 June 2008; accepted 9 October 2008; published 22 April 2009.

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Eprint ID
14855
Resolver ID
CaltechAUTHORS:20090806-133616880

Dates

Created
2009-08-06
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Updated
2021-11-08
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