## The very bright and compact massive young cluster, NGC 3603, has been cited as an example of a starburst in the Milky Way and compared with the much-studied R136/30 Doradus region in the Large Magellanic Cloud. 非常明亮和緻密的大質量年輕星團 NGC 3603 被引用為銀河系中星暴的一個例子，並與大麥哲倫星雲中經過大量研究的 R136/30 劍魚座區域進行了比較。

The O star hinterland of the Galactic starburst, NGC 3603

## The Scutum complex in the inner disk of the Galaxy hosts a number of young clusters and associations of red supergiant stars that are heavily obscured by dust extinction. 銀河系內盤的盾牌複合體擁有許多年輕的星團和紅超巨星組合，這些星團被塵埃滅絕嚴重遮蔽。

Stellar population astrophysics (SPA) with the TNG. GIANO-B spectroscopy of red supergiants in Alicante 7 and Alicante 10.

## We have undertaken a similar analysis for 61 B-type similar targets, towards the young cluster, NGC 346 in the Small Magellanic Cloud (SMC). 我們針對小麥哲倫星雲 (SMC) 中的年輕星團 NGC 346 對 61 個 B 型類似目標進行了類似分析。

The NGC 346 massive star census. Nitrogen abundances for apparently single, narrow lined, hydrogen core burning B-type stars

## 1 Msun not associated with a young cluster. 1 Msun 未與年輕集群關聯。

WISE2150-7520AB: A very low mass, wide co-moving brown dwarf system discovered through the citizen science project Backyard Worlds: Planet 9.

## It is shown that the shallow, power-law density profiles characteristic of young clusters is predicted by the hierarchical star formation scenario. 結果表明，年輕星團的淺冪律密度分佈特徵是由分層恆星形成情景預測的。

The Role of Stellar Feedback in Star Cluster Formation

## In this work we report the discovery of a young cluster of asteroids that originated by the breakup of an asteroid member of the (221)Eos family. 在這項工作中，我們報告了一個年輕的小行星集群的發現，該集群起源於 (221)Eos 家族的一個小行星成員的解體。

Discovery of a young subfamily of the (221) Eos asteroid family

## (abridged) NGC6530 is a young cluster with a complex morphology and star-formation history. （節略）NGC6530 是一個年輕的星團，具有復雜的形態和恆星形成歷史。

Wide-area photometric and astrometric (Gaia DR2) study of the young cluster NGC 6530

## W40 is a blistered Hii region, and Serpens South is an infrared dark cloud accompanied by a young cluster. W40 是一個起泡的 Hii 區域，Serpens South 是一個紅外暗雲，伴隨著一個年輕的星團。

Cluster formation in the W 40 and Serpens South complex triggered by the expanding H ii region