This tightly bound pair of stars lies roughly 1,470 light-years away in the direction of the Vela Constellation.
, scientists are keen to image star growth in order to have a better understanding of how some stars gain so much mass. The derived information may enable them to model the growth process of the Sun.. These stars are actively consuming the surrounding material to stimulate their growth.
Another stunning feature of the image is the presence of two-sided lobes extending outward from the center of the actively forming stars. The image depicts this characteristic in a blazing orange hue. The lobes are inferred to be composed of stellar material emitted by the two central stars., the objects undergo a process of ingesting and ejecting stellar material repeatedly.
Furthermore, the blue strings attention to the most recent ejections from Herbig-Haro 46/47s. These are located at the 2 o'clock position, just below the red horizontal diffraction spike.
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