Very-high-energy γ -Ray Emission from Young Massive Star Clusters in the Large Magellanic Cloud

The Tarantula Nebula in the Large Magellanic Cloud is known for its high star formation activity. At its center lies the young massive star cluster R136, providing a significant amount of the energy that makes the nebula shine so brightly at many wavelengths. Recently, young massive star clusters ha...

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Bibliographic Details
Main Authors:	Aharonian, F, Benkhali, FA, Aschersleben, J, Ashkar, H, Backes, M, Martins, VB, Batzofin, R, Becherini, Y, Berge, D, Bernlöhr, K, Böttcher, M, Bolmont, J, de Bony de Lavergne, M, Borowska, J, Brose, R, Brown, A, Brun, F, Bruno, B, Burger-Scheidlin, C, Casanova, S, Celic, J, Cerruti, M, Chand, T, Chandra, S, Cotter, G
Format:	Journal article
Language:	English
Published:	American Astronomical Society 2024

Very-high-energy γ -Ray Emission from Young Massive Star Clusters in the Large Magellanic Cloud

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