We present a study of the velocity profiles of the v=1-0 S(1) transition of molecular hydrogen (H2) towards the star forming region of OMC-1. A three dimensional data cube is presented which displays the spatial distribution as well as the velocity structure of the H2 emission. A brief description of the data acquisition, reduction and analysis is given.
|Title of host publication||In: Procs of Tridimensional Optical Spectroscopic Methods in Astrophysics, ASP Conference Series 71|
|Publisher||Astronomical Society of the Pacific|
|Publication status||Published - 1995|