Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space

Superwinds and superbubbles driven by mechanical feedback from super star clusters (SSCs) are common features in many star-forming galaxies. While the adiabatic fluid model can well describe the dynamics of superwinds, several observations of starburst galaxies revealed the presence of compact regio...

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Veröffentlicht in:	The Astrophysical journal 2021-11, Vol.921 (1), p.91
Hauptverfasser:	Danehkar, Ashkbiz, Oey, M. S., Gray, William J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Adiabatic flow Astronomical models Astrophysics Cooling Cooling flows Cooling flows (astrophysics) Density Emission line galaxies Galaxies H II regions Hydrodynamics Ionization Kinetic heating Lyman-alpha galaxies Lyman-break galaxies Metallicity Nonequilibrium ionization Outflow Parameters Photoionization Radiation Radiative cooling Star clusters Star formation Star forming regions Starburst galaxies Superbubbles Superclusters
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