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Radiative transfer models of mid-infrared H2O lines in the Planet-forming Region of Circumstellar Disks
R. Meijerink, K. M. Pontoppidan, G. A. Blake +2
The study of warm molecular gas in the inner regions of protoplanetary disks is of key importance for the study of planet formation and especially for the transport of H2O and orga…
A new raytracer for modeling AU-scale imaging of lines from protoplanetary disks
Klaus M. Pontoppidan, Rowin Meijerink, Cornelis P. Dullemond +1
The material that formed the present-day Solar System originated in feeding zones in the inner Solar Nebula located at distances within ~20 AU from the Sun, known as the planet-for…
The Evolution of Massive YSOs in the LMC: Part I. Identification and Spectral Classification
Jonathan P. Seale, Leslie W. Looney, You-Hua Chu +5
We present and categorize Spitzer IRS spectra of 294 objects in the Large Magellanic Cloud (LMC) to create the largest and most complete catalog of massive young stellar object (YS…
High Resolution Spectroscopy of [NeII] Emission from AA Tau and GM Aur
Joan R. Najita, Greg W. Doppmann, Martin A. Bitner +8
We present high resolution (R=80,000) spectroscopy of [NeII] emission from two young stars, GM Aur and AA Tau, which have moderate to high inclinations. The emission from both sour…