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.

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.

是 剑鱼座 的一個 星系。 维基共享资源 上的相關多媒體資源： NGC 1846 NED – NGC 1846 SEDS – NGC 1846 SIMBAD – NGC 1846 VizieR – NGC 1846

2011年11月22日 · Compass and Scale An astronomical image with a scale that shows how large an object is on the sky, a compass that shows how the object is oriented on the sky, and the filters with which the image was made.

NGC 1846 is a globular cluster containing hundreds of thousands of stars in the outer halo of the Large Magellanic Cloud. It was discovered on November 6, 1826,...

2008年5月21日 · Aims: We investigate the change in the surface abundance of 12 C during the evolution along the AGB, aiming to constrain third dredge-up models. Methods: High-resolution, near-infrared spectra of a sample of AGB stars in the LMC cluster NGC 1846 were obtained.

2009年3月26日 · The Advanced Camera for Surveys on board the Hubble Space Telescope has been used to obtain deep, high-resolution images of the intermediate-age star cluster NGC 1846 in the Large Magellanic Cloud. We present new color-magnitude diagrams (CMDs) based on F435W, F555W, and F814W imaging.

2009年5月6日 · In this paper, we conduct a more detailed investigation of NGC 1846 in the LMC than that presented in Mackey et al. ( 2008 ), including the effects of photometric completeness and binary star evolution, new techniques for assessing background contamination, and the radial distribution of cluster stars at different evolutionary phases.

Q1045679 SIMBAD ID: NGC 1846. The following 4 files are in this category, out of 4 total.

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.