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 "a globular cluster, very bright, small, a little extended, stars from 13th to 15th magnitude."

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4000万年的历史 [1] 。

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] 这张照片中最令人惊叹的物体实际上是图像左下角非常小的星团，周围环绕着电离氢（红色）和尘埃（蓝色）的星云。 该 星团 被命名为GALFOR 1，于2018年在哈勃的档案数据中被发现，该数据用于从哈勃望远镜创建这张最新图像。 为了更好地了解这个星团，特别是围绕星团的星云是否也包含 …

2021年7月2日 · 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 Cloud. The cluster – which is in the constellation Tucana (the Toucan) – contains a multitude of stars, many of which are scattered across this striking image.

2021年6月28日 · 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 constellation Tucana (The Toucan) — contains a multitude of stars, many of which are scattered across this striking image.

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 deep space objects compiled by John Louis Emil Dreyer in 1888 to …

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 Magellanic Cloud. NGC 330 is in an age range where the number of post-interaction binaries is predicted to be high near the cluster turnoff (TO).

2022年12月1日 · 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), including a characterization of the stellar content and the estimation of the present-day binary fraction (Bodensteiner et al. 2020, 2021).

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 330 in the Small Magellanic Cloud in order to search for possible imprints of stellar evolution on the multiplicity properties.