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- W3123201765 abstract "Hu,1-2 is a planetary nebula that contains an isolated knot located northwestern of the main nebula, which could be related to a collimated outflow. We present a subsarcsecond H$alpha$+[N,{sc ii}] image and a high-resolution, long-slit spectrum of Hu,1-2 that allow us to identify the southeastern counterpart of the northwestern knot and to establish their high velocity ($>$ 340 km,s$^{-1}$), collimated bipolar outflow nature. The detection of the northwestern knot in POSS red plates allows us to carry out a proper motion analysis by combining three POSS red plates and two narrow-band H$alpha$+[N,{sc ii}] CCD images, with a time baseline of $simeq$ 57 yr. A proper motion of 20 $pm$ 6,mas,yr$^{-1}$ along position angle 312$^{circ}$ $pm$ 15$^{circ}$, and a dynamical age of 1375$^{+590}$llap{$_{-320}$},yr are obtained for the bipolar outflow. The measured proper motion and the spatio-kinematical properties of the bipolar outflow yield a lower limit of 2.7,kpc for the distance to Hu,1-2." @default.
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- W3123201765 date "2012-02-07" @default.
- W3123201765 modified "2023-10-13" @default.
- W3123201765 title "The collimated outflows of the planetary nebula Hu 1-2: proper motion and radial velocity measurements<sup>★</sup>" @default.
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- W3123201765 doi "https://doi.org/10.1111/j.1365-2966.2012.20423.x" @default.
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