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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 1.

Three-color composite of H-band (blue), S(1) line emission (green), and K-band (red) UKIRT WFCAM images of the Serpens South MHO 3252 Y3 region, obtained in 2016 and 2017. Shock-excited features show up in green. MHO 3252 Y3 is the source of a large-scale well-developed bipolar outflow. Proper-motion vectors based on the 2011 Calar Alto data of Teixeira et al. (2012) and on 2016 UKIRT data are indicated.

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