Ou4: a huge, extended and faint bipolar outflow only ~ 700 parsecs distant

ou4_colourreduced_corradi
Image credit: Romano Corradi/(Instituto de Astrofísica de Canarias). Text by the incomparable Astronomy Picture of the Day (APOD) where I recommend you go for links to further web material concerning the discovery.

This nebula is very faint, but also very large in planet Earth’s sky. In the mosaic image, composed with narrowband data from the 2.5 meter Isaac Newton Telescope, it spans some 2.5 full moons toward the constellation Cepheus. Recently discovered by French astro-imager Nicolas Outters, the remarkable nebula’s bipolar shape and emission are consistent with it being a planetary nebula (PN), the gaseous shroud of a dying sun-like star, but its actual distance and origin are unknown. A new investigation suggests Ou4 really lies within the emission region SH2-129 some 2,300 light-years away. Consistent with that scenario, the cosmic squid would represent a spectacular outflow of material driven by a triple system of hot, massive stars, cataloged as HR 8119, seen near the center of the nebula. If so, this truly giant squid nebula would physically be nearly 50 light-years across.

Ou4 might be one of the nearest planetary nebulae although the discoverers caution its nature is not yet fully established. The morphology does seem quite clear from the beautiful image. If the scenario given by Corradi et al. (2014) is correct though, Ou4 is not a PN, as the central object(s) are not sufficiently evolved and in no way like the central stars of true planetary nebulae. [my italics]

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