Red supergiants around the obscured open cluster Stephenson 2
I. Negueruela, A. Marco, C. Gónzalez-Fernández, F. Jiménez-Esteban, J. S. Clark, M. García, E. Solano
Abstract
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I. Negueruela, A. Marco, C. Gónzalez-Fernández, F. Jiménez-Esteban, J. S. Clark, M. García, E. Solano
Abstract
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Context. Several clusters of red supergiants have been discovered in a small region of the Milky Way close to the base of the Scutum-Crux Arm and the tip of the Long Bar. Population synthesis models indicate that they must be very massive to harbour so many supergiants. Amongst these clusters, Stephenson 2, with a core grouping of 26 red supergiants, is a strong candidate to be the most massive young cluster in the Galaxy.
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Context. Several clusters of red supergiants have been discovered in a small region of the Milky Way close to the base of the Scutum-Crux Arm and the tip of the Long Bar. Population synthesis models indicate that they must be very massive to harbour so many supergiants. Amongst these clusters, Stephenson 2, with a core grouping of 26 red supergiants, is a strong candidate to be the most massive young cluster in the Galaxy.
Key concepts: Red supergiant, Supergiant, Context (archaeology), Blue supergiant, Milky Way, Astronomy, Astrophysics, Galaxy