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Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST*
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DOI：10.3847/1538-4357/ae56e8.png)
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Abstract
En 中文
The Antennae galaxies merger produces the brightest infrared emission of any galaxy within ≈20 Mpc, mostly from intense star formation taking place in supergiant molecular cloud complexes in the overlap region. Here, we present new, high-resolution NIRCam and MIRI images of the Antennae galaxies taken with the F150W, F187N, F335M, F360M, F410M, and F770W filters on JWST to search for the predicted but as-yet-undiscovered population of deeply embedded, optically obscured star clusters. We identify a population of 45 sources, 40 previously unknown, with high Brα/Hα and Paα/Hα flux ratios, which are likely very young clusters still embedded or just emerging from their natal cocoons, and estimate their age, extinction (AV), and mass. We find that all are extremely young (≲2.5 Myr), have AV between 2 and 10 mag, and masses between ≈104 and several ×106 M⊙. We believe we have now uncovered all clusters with M ≳ 3 × 104 M⊙ and AV ≳ 2 mag in the Antennae. While our sample represents a small fraction (≈15%) of clusters younger than 3 Myr by number, it dominates the ionizing photon luminosity across the galaxy pair (≈60%). We find elevated H2/polycyclic aromatic hydrocarbon ratios of the interstellar medium surrounding the most massive pair of embedded clusters, supporting the idea that merger-induced shock-heated gas plays an important role in the formation of extremely massive clusters.
Keywords:
Young star clusters
Embedded clusters
Antennae galaxies
JWST observations
Star formation
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