Celestial hemisphere:  Southern  ·  Constellation: Puppis (Pup)  ·  Contains:  NGC 2467
NGC 2467 in H alpha, Lawrence E. Hazel
NGC 2467 in H alpha
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NGC 2467 in H alpha

NGC 2467 in H alpha, Lawrence E. Hazel
NGC 2467 in H alpha
Powered byPixInsight

NGC 2467 in H alpha

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Description

NGC 2467 is a star-forming region, known popularly as the "Skull and Crossbones nebula" whose appearance has occasionally also been likened to that of a colorful mandrill. It includes areas where large clouds of hydrogen gas incubate new stars. This region was one of the areas featured in the book Hubble’s Universe: Greatest Discoveries and Latest Images by Terence Dickinson.

Involved in the nebula are two very young star clusters, Haffner 18 and 19 which have formed from the abundant gas and dust in the region. Haffner 18 is an open star cluster that lies in the center of the emission nebula NGC 2467, some 19,200 light-years from Earth in the Puppis Milky Way. Its age is somewhat controversial, some considering it to be as young as only 1 million years. Haffner 18 contains about 50 stars, among which include several short lived masssive examples. These massive stars are surrounded by a small dense shell of hydrogen cataloged as Wray 15-101 which is about 2.5 light years in diameter and expands at a speed of about 20 kilometers per second. It possibly was created about 40,000 years ago.

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