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Forming an Early O-type Star Through Gas Accretion?
Luis A. Zapata, Aina Palau, Paul Ho +4
We present high angular resolution ( 3) and sensitive 1.3 mm continuum, cyanogen (CN) and vinyl cyanide (CHCN) line observations made with the Submillimeter Array…
A dense micro-cluster of Class 0 protostars in NGC 2264 D-MM1
Paula S. Teixeira, Luis A. Zapata, Charles J. Lada
We present sensitive and high angular resolution (~1") 1.3 mm continuum observations of the dusty core D-MM1 in the Spokes cluster in NGC 2264 using the Submillimeter Array. A dens…
Circumbinary Molecular Rings Around Young Stars in Orion
Luis A. Zapata, Paul T. P. Ho, Luis F. Rodriguez +2
We present high angular resolution 1.3 mm continuum, methyl cyanide molecular line, and 7 mm continuum observations made with the Submillimeter Array and the Very Large Array, towa…
Large Scale Flows from Orion-South
W. J. Henney, C. R. O'Dell, Luis A. Zapata +3
Multiple optical outflows are known to exist in the vicinity of the active star formation region called Orion-South (Orion-S). We have mapped the velocity of low ionization feature…