Evolution of clouds in radio galaxy cocoons

Details Evolution of clouds in radio galaxy cocoons Evolution of clouds in radio galaxy cocoons

2002-09-28

arxiv.org/abs/astro-ph/0209601v1

Astron.Astrophys. 395 (2002) L13-L16

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, movies available at http://www.strw.leidenuniv.nl/TheoryGroup/IG-Cloud.html

Scientific paper

10.1051/0004-6361:20021408

This letter presents a numerical study of the evolution of an emission line cloud of initial density 10 cm$^{-3}$, temperature $10^4$ K, and size 200 pc, being overtaken by a strong shock wave. Whereas previous simple models proposed that such a cloud would either be completely destroyed, or simply shrink in size, our results show a different and more complex behaviour: due to rapid cooling, the cloud breaks up into many small and dense fragments, which can survive for a long time. We show that such rapid cooling behaviour is in fact expected for a wide range of cloud and shock properties. This process applies to the evolution of emission line clouds being overtaken by the cocoon of a radio jet. The resulting small clouds would be Jeans unstable, and form stars. Our results thus give theoretical credibility to the process of jet induced star formation, one of the explanations for the alignment of the optical/UV and radio axis observed in high redshift radio galaxies.

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