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http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/2257| Young Stellar Clusters with a Schuster Mass Distribution - I: Stationary Winds | |
| SERGIO MARTINEZ GONZALEZ SERGIY SILICH GUILLERMO TENORIO TAGLE | |
| Acceso Abierto | |
| Atribución-NoComercial-SinDerivadas | |
| Stars: winds, outflows Galaxies: star clusters: general Galaxies: starburst Hydrodynamics Instabilities | |
| Hydrodynamic models for spherically-symmetric winds driven by young stellar clusters with a generalized Schuster stellar density profile are explored. For this we use both semi-analytic models and 1D numerical simulations. We determine the properties of quasi-adiabatic and radiative stationary winds and define the radius at which the flow turns from subsonic into supersonic for all stellar density distributions. Strongly radiative winds diminish significantly their terminal speed and thus their mechanical luminosity is strongly reduced. This also reduces their potential negative feedback into their host galaxy ISM. The critical luminosity above which radiative cooling becomes dominant within the clusters, leading to thermal instabilities which make the winds non-stationary, is determined, and its dependence on the star cluster density profile, core radius and half mass radius is discussed. | |
| The Astrophysical Journal | |
| 31-05-2013 | |
| Artículo | |
| Inglés | |
| Estudiantes Investigadores Público en general | |
| Palous, Jan., et al., (2013). Young Stellar Clusters with a Schuster Mass Distribution - I: Stationary Winds, The Astrophysical Journal, Vol. 772(2):1-21 | |
| ASTRONOMÍA Y ASTROFÍSICA | |
| Versión aceptada | |
| acceptedVersion - Versión aceptada | |
| Aparece en las colecciones: | Artículos de Astrofísica |
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| 38. Young Stellar Clusters with a Shuster Mass Distribution – I - Stationary Winds.pdf | 418.09 kB | Adobe PDF | Visualizar/Abrir |