
NGC 3597 - Wikipedia
NGC 3597 is a galaxy located approximately 150 million light-years away in the constellation of Crater. [2][3] It was discovered by John Herschel on March 21, 1835. [4] NGC 3597 is thought …
NGC 3597 - 维基百科,自由的百科全书
NGC 3597 是一个位于 巨爵座 的 星系,距离地球1.5亿光年,1835年3月21日由 約翰·赫歇爾 发现 [2][3][4]。 NGC 3597可能由两个大星系碰撞产生,日后可能会发展成 椭圆星系 [5][6]。
NGC 3597 - 維基百科,自由的百科全書 - zh.wikipedia.org
NGC 3597 是一個位於 巨爵座 的 星系,距離地球1.5億光年,1835年3月21日由 約翰·赫歇爾 發現 [2][3][4]。 NGC 3597可能由兩個大星系碰撞產生,日後可能會發展成 橢圓星系 [5][6]。
Hubble Views a Galactic Mega-merger - NASA Science
2016年1月15日 · The subject of this NASA/ESA Hubble Space Telescope image is known as NGC 3597. It is the product of a collision between two good-sized galaxies, and is slowly …
A galactic mega-merger | ESA/Hubble
2016年1月11日 · The subject of this NASA/ESA Hubble Space Telescope image is known as NGC 3597. It is the product of a collision between two good-sized galaxies, and is slowly …
Imaging of the merging galaxy NGC 3597 and its population of ...
Abstract: We present wide field-of-view near-infrared imaging from the NTT and very deep optical imaging from the HST of the young merging galaxy NGC 3597. The morphology of the galaxy …
Globular cluster formation in merging galaxies? - NASA Technical ...
1993年1月1日 · NGC 3597 is an advanced merger which has already developed into an elliptical-like object with a de Vaucouleurs brightness distribution, but intense star formation is …
[astro-ph/9910421] Imaging of the Merging Galaxy NGC 3597 …
1999年10月22日 · We present wide field-of-view near-infrared imaging from the NTT and very deep optical imaging from the HST of the young merging galaxy NGC 3597. The morphology …
Imaging of the merging galaxy NGC 3597 and its population of ...
We present wide field-of-view near-infrared imaging from the NTT and very deep optical imaging from the HST of the young merging galaxy NGC 3597. The morphology of the galaxy and the …
NGC 3597: Hubble Captures Young Merging Galaxy - Sci.News
2016年1月11日 · According to scientists, NGC 3597 is the result of a recent merger between two near equal mass spiral galaxies, at least one of which contained a strong bulge. The galaxy is …