Gas lines from the 5-Myr old optically thin disk around HD 141569A Herschel observations and modeling

@article{Thi2013GasLF,
  title={Gas lines from the 5-Myr old optically thin disk around HD 141569A Herschel observations and modeling},
  author={W. Thi and C. Pinte and E. Pantin and J. Augereau and G. Meeus and F. M{\'e}nard and C. Martin-Zaidi and P. Woitke and P. Rivi{\`e}re-Marichalar and I. Kamp and A. Carmona and G. Sandell and C. Eiroa and W. Dent and B. Montesinos and G. Aresu and R. Meijerink and M. Spaans and G. White and D. Ardila and J. Lebreton and I. Mendigutia and S. Brittain},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={561}
}
Context. The gas- and dust dissipation processes in disks around young stars remain uncertain despite numerous studies. At the distance of∼ 99‐116 pc, HD141569A is one of the nearest HerbigAe stars that is surrounded by a tenuous disk, probably in transition between a massive primordial disk and a debris disk. Atomic and molecular gases haves been found in the structured 5-Myr old HD141569A disk, making HD141569A the perfect object within which to directly study the gaseous atomic and molecular… Expand
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