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The Temperature and Ionization of T-Tauri Micro-Jets

  • Darren M. O’Brien
  • Paulo J. V. Garcia
  • Jonathan Ferreira
  • Sylvie Cabrit
  • Luc Binette
Chapter

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

ISM: jets and outflows stars: pre-main sequence MHD line profiles accretion disks coronae 

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Copyright information

© Springer Science+Business Media Dordrecht 2004

Authors and Affiliations

  • Darren M. O’Brien
    • 1
  • Paulo J. V. Garcia
    • 2
  • Jonathan Ferreira
    • 3
  • Sylvie Cabrit
    • 4
  • Luc Binette
    • 5
  1. 1.Centro de Astrofísica da Universidade do Porto & Departamento de Matemática Aplicada da Faculdade de Ciências do PortoPortugal
  2. 2.Centro de Astrofísica da Universidade do Porto & Faculdade de Engenharia da Universidade do PortoPortugal
  3. 3.Laboratoire d’Astrophysique de GrenobleFrance
  4. 4.Observatoire de ParisLERMAFrance
  5. 5.Instituto de AstronomíaCiudad UniversitariaMexico

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