Hub-Filament Structure and Star Formation in OMC1
Date:
Abstact: We have observed the Orion Molecular Cloud 1 region using the Submillimeter array (SMA) and the 10.4 m telescope of the Caltech Submillimeter Observatory (CSO) with the N2H+ 3-2 line. The N2H+ 3-2 line is a suitable tracer of high density gas, the structure and kinematics of which are directory related to star formation. In this project, I work on combining the interferometer (SMA) and single-dish (CSO) data of N2H+.