T-Tauri-star

Figure 2: A model of a T Tauri star with an accretion disk. The Doppler effect seen in the emission line spectra are shown below consistent with one jet projected towards us and one away. The stellar wind is powered by the rotation of the system through the poles. From page 473 of Carroll & Ostlie (1st Ed.).

By John Gideon Hartnett

Dr John G. Hartnett is an Australian physicist and cosmologist, and a Christian with a biblical creationist worldview. He received a B.Sc. (Hons) and Ph.D. (with distinction) in Physics from The University of Western Australia, W.A., Australia. He was an Australian Research Council (ARC) Discovery Outstanding Researcher Award (DORA) fellow at the University of Adelaide, with rank of Associate Professor. Now he is retired. He has published more than 200 papers in scientific journals, book chapters and conference proceedings.

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