
NGC 1792 - Wikipedia
NGC 1792 is a spiral galaxy located in the southern Columba constellation. It was discovered by Scottish astronomer James Dunlop on October 4, 1826. This galaxy is located at a distance of about 36.4 million light-years and is receding from the Milky Way with a heliocentric radial velocity of 1,208 km/s. [ 3 ]
The Stellar Forge - ESA/Hubble
2020年12月7日 · An orange glow radiates from the centre of NGC 1792, the heart of this stellar forge. Captured by the NASA/ESA Hubble Space Telescope, this intimate view of NGC 1792 gives us some insight into this galactic powerhouse. The vast swathes of tell-tale blue seen throughout the galaxy indicate areas that are full of young, hot stars, and it is in ...
Hubble Sees a Stellar Furnace - NASA Science
2021年2月5日 · Captured by the NASA/ESA Hubble Space Telescope, this intimate view of NGC 1792 gives us some insight into this galactic powerhouse. The vast swathes of tell-tale blue seen throughout the galaxy indicate areas that are full of young, hot stars, and it is in the shades of orange, seen nearer the center, that the older, cooler stars reside.
NGC 1792 - 维基百科,自由的百科全书 - zh.wikipedia.org
NGC 1792 是 天鸽座 的一个 星系。 维基共享资源 上的相关多媒体资源: NGC 1792.
Hubble Images Beautiful Star-Forming Spiral Galaxy: NGC 1792
2020年12月7日 · This Hubble image shows NGC 1792, a spiral galaxy 36.4 million light-years away in the southern constellation of Columba. The vast swathes of tell-tale blue seen throughout NGC 1792 indicate areas that are full of young, hot stars, and it is in the shades of orange, seen nearer the center that the older, cooler stars reside.
NGC 1792: A galactic powerhouse - Earth.com
2025年2月5日 · Today’s Image of the Day from the European Space Agency features NGC 1792, a spiral galaxy located in the constellation Columba about 43 million light-years away from Earth. This galaxy, discovered by British astronomer James Dunlop in 1826, is part of the larger NGC 1808 group of galaxies.
NGC 1792: A beautiful tapestry of contrasting colour
2022年6月16日 · This dense, swirling spiral galaxy is NGC 1792, located 34.6 million light years away in the constellation of Columba, the Dove. This crystal-clear image from the Hubble Space Telescope shows a red core of older stars and spiral arms of sparkling young blue stars, interwoven with dark lanes of dust.
Hubble Sees A Stellar Furnace - SpaceNews
2021年2月7日 · Captured by the NASA/ESA Hubble Space Telescope, this intimate view of NGC 1792 gives us some insight into this galactic powerhouse. The vast swathes of tell-tale blue seen throughout the...
The distribution and nature of star formation regions in NGC 1792
1994年9月10日 · A strong asymmetry with respect to the major axis has been found in the spatial distribution of H II regions in NGC 1792 detected on our H(alpha) image. In the radio continuum, this asymmetry is even stronger than in H(alpha), indicating that supernova activity set in earlier in the northeastern half of the disk than southwest of the nucleus.
NGC 1792 - 百度百科
NGC 1792 是天鸽座的一个星系。