The Temperature and Ionization of T-Tauri Micro-Jets

Details The Temperature and Ionization of T-Tauri Micro-Jets The Temperature and Ionization of T-Tauri Micro-Jets

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.292..609o&link_type=abstract

Astrophysics and Space Science, v. 292, Issue 1, p. 609-617 (2004).

Astronomy and Astrophysics

Astrophysics

Ism: Jets And Outflows, Stars: Pre-Main Sequence, Mhd, Line, Profiles, Accretion Disks, Coronae

Scientific paper

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.

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