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We present new mid-infrared images of the central region of the Orion Nebula using the newly commissioned SOFIA airborne telescope and its 5 -- 40 micron camera FORCAST. The 37.1 micron images represe...
In some massive stars, magnetic fields are thought to confine the outflowing radiatively-driven wind. Although theoretical models and MHD simulations are able to illustrate the dynamics of such a magn...
We present the full results of our 3-year long Submillimeter Array survey of protoplanetary disks in the Orion Nebula Cluster. We imaged 23 fields at 880 microns and 2 fields at 1330 microns, covering...
We present the sub-mm/mm SED for a sample of eight young circumstellar disks in the outer regions of the Orion Nebula Cluster.
Velocity structure in the orion nebula. ii. emission line atlas of partially ionized to fully ionized gas。
The Radial Velocity Profiles of some Proplyds in the Orion Nebula
Determination of the Electron Density in the Orion Nebula with High Spectral Resolution
Temperature and Density Gradients in the Orion Nebula
Density gradients and internal dust in the Orion nebula
Fe II in the orion nebula:spectroscopic observations and theoretical models。
Fluorescence of permitted lines in the orion nebula
Dust in and near the orion nebula     Dust  rion nebula       2009/6/11
Dust in and near the orion nebula
An ionized microjet from the orion nebula proplyd LV 2。
Fabry-perot kinematics of hh 202-204 in the orion nebula:are they part of a big bipolar outflow?
High Velocity Outflows in the Orion Nebula Determined from Proper Motions。

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