HIGHLIGHTS
- who: Rab Ch. and collaborators from the University Observatory, Faculty of Physics, Ludwig-Maximilians-Universitu00e4t Mu00fcnchen, Scheinerstr1, Munich, Germany have published the article: Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models, in the Journal: (JOURNAL)
- what: The authors aim to interpret observational data for molecular hydrogen and atomic oxygen lines that show kinematic disk-wind signatures to investigate whether or not purely thermally driven winds are consistent with the data. The authors aim to interpret observations of spectral lines o-H2 1-0 S(1) at . . .
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