none


NRAO/Socorro Colloquium Series

Jose-Maria Torrelles

CSIC


Short-lived Pulsed Outflow Events in Massive Protostars

VLBI multi-epoch water maser observations are a powerful tool to study the dense, warm shocked gas very close to massive protostars. The very high-angular resolution of these observations allow us to measure the proper motions of the masers in a few weeks, and together with the radial velocity, to determine their full kinematics. In this talk we present a summary of the main VLBA observational results obtained by our group during the last ten years toward the massive star-forming regions of Cepheus A, W75N, and AFGL 2591, among them: (i) the identification of different centers of high-mass star formation activity at scales of 100 AU, unknown previously; and (ii) the discovery of new phenomena associated with the early stages of high-mass protostellar evolution. For example, the identification of the simultaneous presence of a wide-angle outflow and a highly collimated jet in a massive object, similar to what is observed in some low-mass protostars, and the short-lived outflow events that seem to be characteristic of the first stages of evolution of massive protostars. Some of the important implications of these results in the study of high-mass star formation are discussed.


June 28, 2013
11:00 am

Array Operations Center Auditorium

All NRAO employees are invited to attend via video, available in Charlottesville CR  230, Green Bank Auditorium and Tucson N525.

Local Host: Juergen Ott


Connect with NRAO

The NSF National Radio Astronomy Observatory and NSF Green Bank Observatory are facilities of the U.S. National Science Foundation operated under cooperative agreement by Associated Universities, Inc.