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The Temperature and Ionization of T-Tauri Micro-Jets
Authors:Darren M O'Brien  Paulo JV Garcia  Jonathan Ferreira  Sylvie Cabrit  Luc Binette
Institution:1. Centro de Astrofísica da Universidade do Porto & Departamento de Matemática Aplicada da Faculdade de Ciências do Porto, Portugal
2. Laboratoire d'Astrophysique de Grenoble, France
3. LERMA, Observatoire de Paris, France
4. Instituto de Astronomía, Ciudad Universitaria, Mexico
Abstract:The effects of phenomenological heating functions on the flow thermodynamics of cold T-Tauri disk winds are examined. Turbulent dissipation (mechanical) heating and a warm disk corona are invoked to heat the wind. The temperature and ionization evolution are solved for along the flow. The results allow the construction of synthetic observations; emission maps, forbidden line ratios, line fluxes and line profiles; and successfully reproduce a number of observed trends. Mechanical heating produces line ratios and fluxes that fit very well with observations. Invoking a warm disk corona successfully reproduces forbidden line profile low velocity components.
Keywords:
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