Multi Field imaging with the OVRO millimeter array
نویسنده
چکیده
Leonardo Testi1 and Anneila I. Sargent California Institute of Te hnology, MS 105-24, Pasadena, CA 91125 Abstra t. We review some of the basi guidelines used to plan, exe ute and analyse multield observations at the Owens Valley Radio Observatory millimeter wave array. As a working example we dis uss our observations of the inner 50.5 50.5 of the Serpens loud ore. The results of our observations of this protoluster ore suggest that the stellar IMF is determined during the ore fragmentation pro ess.
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