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Variability and Jet Activity in the YSO MHO 3252 Y3 in Serpens South

  • Authors: Klaus W. Hodapp, and Rolf Chini

2018 The Astrophysical Journal 864 172.

  • Provider: AAS Journals

Caption: Figure 8.

Four wavelength channels of the 2015 OSIRIS data in the 20 mas scale, displayed here on 10 mas pixels. These channel images were continuum subtracted, but 10% of the flux of the continuum image has been reinserted at the position of the driving star to identify its position. Even ignoring the BLVC, several areas in the jet show asymmetric features with wavelength that create a rotational component to the velocity field. However, the velocity field is far more complicated than simply a rigid rotation of the microjet.

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