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- W3100016342 abstract "We present observations of CO(3–2) and 13CO(3–2) emission near the supernebula in the dwarf galaxy NGC 5253, which contains one of the best examples of a potential globular cluster in formation. The 03 resolution images reveal an unusual molecular cloud, Cloud D1, that is coincident with the radio-infrared supernebula. The ∼6 pc diameter cloud has a linewidth, Δ v = 21.7 , that reflects only the gravitational potential of the star cluster residing within it. The corresponding virial mass is 2.5 × 105 . The cluster appears to have a top-heavy initial mass function, with M* ≳ 1–2 . Cloud D1 is optically thin in CO(3–2), probably because the gas is hot. Molecular gas mass is very uncertain but constitutes <35% of the dynamical mass within the cloud boundaries. In spite of the presence of an estimated ∼1500–2000 O stars within the small cloud, the CO appears relatively undisturbed. We propose that Cloud D1 consists of molecular clumps or cores, possibly star-forming, orbiting with more evolved stars in the core of the giant cluster." @default.
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- W3100016342 date "2017-09-01" @default.
- W3100016342 modified "2023-10-16" @default.
- W3100016342 title "ALMA Detects CO(3–2) within a Super Star Cluster in NGC 5253" @default.
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- W3100016342 doi "https://doi.org/10.3847/1538-4357/aa8669" @default.
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