NGC 330 is an open cluster in the Small Magellanic Cloud. It is located in the constellation Tucana. It was discovered on 1 August 1826 by James Dunlop. It was described by Dreyer as …

ngc 330 是杜鹃座 小麦哲伦云的一個球狀星團（疏散星团）。它於1826年8月1日由詹姆士·敦洛普發現。約翰·路易·埃米爾·德雷耳認為ngc 330非常明亮，而且体积小。ngc 330大约有4000万 …

这张本周图片描绘了 疏散星团 NGC 330，它位于小麦哲伦星云内部，距离地球约180000光年。 这个星团位于杜鹃座，包含许多恒星，其中许多星星散布在这张引人注目的图像中。 [1] 这张照 …

Jul 2, 2021 · This image taken with the NASA/ESA Hubble Space Telescope depicts the open star cluster NGC 330, which lies around 180,000 light-years away inside the Small Magellanic …

Jun 28, 2021 · This Picture of the Week depicts the open star cluster NGC 330, which lies around 180,000 light-years away inside the Small Magellanic Cloud. The cluster — which is in the …

NGC 330 is a Cluster of Stars located in the constellation of Tucana in the southern hemisphere. NGC 330 is called NGC 330 in the New General Catalogue (NGC). This catalogue is a list of …

Aims: Here, we aim to derive the physical parameters and study the distribution of (projected) rotational velocities of B-type stars in the ∼35 Myr-old, massive cluster NGC 330 in the Small …

Dec 1, 2022 · We will further introduce NGC 330, a young massive star cluster in the SMC (Sect. 5.3), and present a detailed spectroscopic survey of NGC 330 with MUSE (Sect. 5.4), …

NGC 330 Andrew Murrell. NGC330 is one of the brightest clusters in the entire SMC. It is easily visible in a pair of 10X50 binoculars, and can be found 20 arc minutes Southwest of NGC 346.

Aims: Using multi-epoch integral-field spectroscopy, we aim to investigate the multiplicity properties of the massive-star population in the dense core of the ∼40 Myr old cluster NGC …