NGC 2467, nicknamed the "Skull and Crossbones Nebula", [3] is a star-forming region 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. [4]

ngc 2467是一个恒星形成区域，俗称“骷髅头星云”， [1] 其外观偶尔也被比喻为色彩丰富的山魈。它包括含有大量氢气的区域，产生新的恒星。 它包括含有大量氢气的区域，产生新的恒星。

NGC 2467, located in the constellation Puppis, is a spectacular HII region—a vast cloud of gas and dust where new stars are born. Nicknamed the "Skull Nebula" due to its evocative shape, it lies approximately 13,000 light-years from Earth.

NGC 2467是一个船尾座的恒星形成区域，俗称“骷髅头星云”，其外观偶尔也被比喻为色彩丰富的山魈。 它包括含有大量氢气的区域，产生新的恒星。 它是特伦斯·迪金森著作《哈勃的宇宙：最伟大的发现和最新画面》（Hubble’s Universe: Greatest Discoveries and Latest Images）一书中被作为特色描述的区域之一。

2024年2月21日 · This vivid picture of an active star forming region — NGC 2467, otherwise known as the Skull and Crossbones nebula — is as sinister as it is beautiful. This image of dust, gas and bright young stars, gravitationally bound into the form of a grinning skull, was captured with the FORS instrument on ESO’s Very Large Telescope (VLT).

NGC 2467 是一個恆星形成區域，俗稱「骷髏頭星雲」， [1] 其外觀偶爾也被比喻為色彩豐富的 山魈。 它包括含有大量氫氣的區域，產生新的恆星。 [2] 它是特倫斯·迪金森著作《哈勃的宇宙：最偉大的發現和最新畫面》（Hubble’s Universe: Greatest Discoveries and Latest Images）一書中被作為特色描述的區域之一。 [3] [nb 1] NGC 2467曾長期被認為是 船尾座 的核心。 然而，NGC 2467並不指一個特殊的開放星群， [4] 其實，它是由幾個具有明顯不同的距離和明顯不同的徑 …

NGC 2467 is an Open cluster associated with the Emission nebula Sh2-311 with an age of a few million years at most, located some 13 000 – 17 000 light-years away in the southern constellation of Puppis. It is an extremely active stellar nursery, where new stars are born continuously from large clouds of dust and gas.

2018年1月28日 · Name(s): NGC 2467. The Skull and Bones Nebula. Type: Emission Nebula. RA: 07h 52m 33s. Dec: -26º 26’ 48” Constellation: Puppis. Size (arcmin): 14×14. Magnitude: +7.1. Distance: 13,200 ly

2010年7月13日 · A colourful star-forming region is featured in this stunning new NASA/ESA Hubble Space Telescope image of NGC 2467. Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars.

This remarkable emission nebula was discovered by William Herschel in 1784. He classified it as a planetary nebula, simply because of its rounded shape. However, today we use Herschel's term Planetary...