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Volume 625 Issue 7993, 4 January 2024

Growth factor

The cover shows an artist’s impression of a massive young star in the process of forming. Around it is a disk-like structure of gas and dust from which the star accretes matter for its further growth. Associated with the accretion process, the star is also launching a powerful bipolar jet. All of the direct detections of disks around massive young stars are in the Milky Way, but in this week’s issue, Anna McLeod and colleagues present the discovery of an accretion disk around a massive young star in our nearest neighbouring galaxy, the Large Magellanic Cloud. The researchers’ observations suggest that there is a rotating toroid feeding the accretion disk and thus the growth of the star. Unlike other such young stars, this star can be detected optically, a consequence of the fact that it is developing in a region with low dust content and low metallicity.

Cover image: ESO/M. Kornmesser.

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