On the Rapidly Cooling Interior of Supergalactic Winds

Bibcode
2003ApJ...590..791S
DOI
10.1086/375133
Silich, S.; Tenorio-Tagle, G.; Muñoz-Tuñón, C.
Referencia bibliográfica

The Astrophysical Journal, Volume 590, Issue 2, pp. 791-796.

Fecha de publicación:
6
2003
Revista
The Astrophysical Journal
Número de autores
3
Número de autores del IAC
1
Número de citas
64
Número de citas referidas
55
Descripción
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.
Tipo
Con árbitro
Galaxias
Métodos

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