Protostars and Planets VI, Heidelberg, July 15-20, 2013
Gould Belt Origin
Rivera, Leticia (CRyA)
Loinard, Laurent (CRyA)
Dzib, Sergio (CRyA)
Using archive VLA data and recent observations on the Karl G. Jansky Very Large Array it is worked on a semi-automatic python/CASA code to select, reduce and plot several young stars belonging to the Ophiuchus core. This code mean to help to select observations made along the 30 years of the VLA done in the selected area with the wide configurations A and B, and in the X and C band, to determine their position and compare it with the most recent ones. In this way it is possible to determinate their proper motion with very high precision.
It is presented the phases of the process and our first results worked on three well know stars: S1, DoAr 21 and VLA1623.
This is the tip of a bigger work that includes Taurus molecular cloud and other important recent star formation regions belonging to the Gould Belt. Our goal is to support the most suitable among several theories about Gould Belt origin or provide a new one taking in count the dynamics of those regions.
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