Bibcode
DOI
Silich, S.; Tenorio-Tagle, G.; Muñoz-Tuñón, C.
Bibliographical reference
The Astrophysical Journal, Volume 590, Issue 2, pp. 791-796.
Advertised on:
6
2003
Journal
Citations
62
Refereed citations
52
Description
Here we present the steady-state numerical solution and two-dimensional
hydrodynamic calculations of supergalactic winds, taking into
consideration strong radiative cooling. The two possible outcomes:
quasi-adiabatic and strongly radiative flows, are thoroughly discussed,
together with their implications on the appearance of supergalactic
winds in both the X-ray and visible line regimes.