Celestial hemisphere:  Southern  ·  Constellation: Carina (Car)  ·  Contains:  HD302609  ·  HD302610  ·  HD302611  ·  HD302612  ·  HD302613  ·  HD302614  ·  HD302615  ·  HD302618  ·  HD302619  ·  HD302620  ·  HD302623  ·  HD302624  ·  HD302656  ·  HD302661  ·  HD302662  ·  HD302663  ·  HD302664  ·  HD302665  ·  HD302666  ·  HD302668  ·  HD302669  ·  HD302670  ·  HD302682  ·  HD302683  ·  HD89358  ·  HD89359  ·  HD89646  ·  HD89725  ·  HD89756  ·  HD89769  ·  And 1 more.
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NGC 3199 – The fault lies not in our Wolf-Rayet star, Charles Pevsner
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NGC 3199 – The fault lies not in our Wolf-Rayet star

Getting plate-solving status, please wait...
NGC 3199 – The fault lies not in our Wolf-Rayet star, Charles Pevsner
Powered byPixInsight

NGC 3199 – The fault lies not in our Wolf-Rayet star

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Description

Usually a massive, hot Wolf-Rayet star blasts away surrounding molecular gases and other interstellar debris more or less equally in all directions, forming a roughly spherical bubble.  This hasn’t happened here; WR-18, also known by the catchy designation HD89358, has selectively sculpted a distinctive banana-shaped arc in one direction.  Early studies of this nebula attributed the cause to bow shock, as a fast-moving WR-18 plows through interstellar material.  However, a more recent 2017 study presents evidence that it’s just dense material that has clumped up, like an area rug on a slippery floor, and WR-18 is not in fact a runaway star heedlessly barging into molecular clouds.

This image is cropped from a 2-panel mosaic.

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NGC 3199 – The fault lies not in our Wolf-Rayet star, Charles Pevsner