NGC 1846 is a globular cluster containing hundreds of thousands of stars in the outer halo of the Large Magellanic Cloud. [3] It was discovered on November 6, 1826, by James Dunlop and is included in the New General Catalogue .

ngc 1846 是剑鱼座的一个星系。 维基共享资源上的相关多媒体资源：ngc 1846. ned – ngc 1846; seds – ngc 1846; simbad – ngc 1846; vizier – ngc 1846

2011年11月22日 · A new NASA Hubble Space Telescope image shows globular cluster NGC 1846, a spherical collection of hundreds of thousands of stars in the outer halo of the Large Magellanic Cloud, a neighboring dwarf galaxy of the Milky Way that can be seen from the southern hemisphere.

2011年11月22日 · A new NASA Hubble Space Telescope image shows globular cluster NGC 1846, a spherical collection of hundreds of thousands of stars in the outer halo of the Large Magellanic Cloud, a neighboring dwarf galaxy of the Milky Way that can be seen from the southern hemisphere.

We present a detailed study of stellar rotation in the massive 1.5 Gyr old cluster NGC 1846 in the Large Magellanic Cloud. Similar to other clusters at this age, NGC 1846 shows an extended main-sequence turn-off (eMSTO), and previous photometric …

2013年2月9日 · NGC 1846 and NGC 1783 are two massive star clusters in the Large Magellanic Cloud, hosting both an extended main-sequence turn-off and a dual clump of red giants. They present similar masses but differ mainly in angular size.

I have not observed NGC 1846. I obtained the calibrated lights frames used to create the final image from iTelescope.com. The frames were imaged by the T59 telescope at the Siding Spring Observatory ...

2007年6月20日 · We report on Hubble Space Telescope /ACS photometry of the rich intermediate-age star cluster NGC 1846 in the Large Magellanic Cloud, which clearly reveals the presence of a double main-sequence turn-off in this object.

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2022年7月28日 · In this work, we focus on NGC 1846, which belongs to the category of massive (≳10 4 M ⊙), intermediate-age (∼ 1−2 Gyr) clusters that reside in the Magellanic Clouds (Bastian & Niederhofer 2015, hereafter BN15). Like other clusters, it offers an opportunity to tune a model of stellar structure and evolution simultaneously to all of its ...