Abstract
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.
Original language | English |
---|---|
Title of host publication | In: Procs of Tridimensional Optical Spectroscopic Methods in Astrophysics, ASP Conference Series 71 |
Publisher | Astronomical Society of the Pacific |
Pages | 173-181 |
ISBN (Print) | 0-937707-90-2 |
Publication status | Published - 1995 |