Abstract

We are conducting a Jansky Very Large Array (VLA) Ka-band (8 mm and 1 cm) and C-band (4 cm and 6.4 cm) survey of all known protostars in the Perseus Molecular Cloud, providing resolution down to similar to 0 ''.06 and similar to 0 ''.35 in the Ka band and C band, respectively. Here we present first results from this survey that enable us to examine the source NGC 1333 IRAS2A in unprecedented detail and resolve it into a protobinary system separated by 0 ''.621 +/- 0 ''.006 (similar to 143 AU) at 8 mm, 1 cm, and 4 cm. These two sources (IRAS2A VLA1 and VLA2) are likely driving the two orthogonal outflows known to originate from IRAS2A. The brighter source IRAS2A VLA1 is extended perpendicular to its outflow in the VLA data, with a deconvolved size of 0 ''.055 (similar to 13 AU), possibly tracing a protostellar disk. The recently reported candidate companions (IRAS2A MM2 and MM3) are not detected in either our VLA data, Combined Array for Research in Millimeter-wave Astronomy (CARMA) 1.3 mm data, or Submillimeter Array (SMA) 850 mu m data. SMA CO (J = 3 -> 2), CARMA CO (J = 2 -> 1), and lower-resolution CARMA CO (J = 1 -> 0) observations are used to examine the outflow origins and the nature of the candidate companions to IRAS2A VLA1. The CO (J = 3 -> 2) and (J = 2 -> 1) data show that IRAS2A MM2 is coincident with a bright CO emission spot in the east west outflow, and IRAS2A MM3 is within the north south outflow. In contrast, IRAS2A VLA2 lies at the east west outflow symmetry point. We propose that IRAS2A VLA2 is the driving source of the east west outflow and a true companion to IRAS2A VLA1, whereas IRAS2A MM2 and MM3 may not be protostellar.