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Time Evolution Images of the Hypergiant RW Cephei during the Rebrightening Phase Following the Great Dimming

Stars with initial masses larger than 8 M _⊙ undergo substantial mass loss through mechanisms that remain elusive. Unraveling the origins of this mass loss is important for comprehending the evolutionary path of these stars, the type of supernova explosion, and whether they become neutron stars or b...

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I tiakina i:
Ngā kaituhi matua: Narsireddy Anugu, Douglas R. Gies, Rachael M. Roettenbacher, John D. Monnier, Miguel Montargés, Antoine Mérand, Fabien Baron, Gail H. Schaefer, Katherine A. Shepard, Stefan Kraus, Matthew D. Anderson, Isabelle Codron, Tyler Gardner, Mayra Gutierrez, Rainer Köhler, Karolina Kubiak, Cyprien Lanthermann, Olli Majoinen, Nicholas J. Scott, Wolfgang Vollmann
Hōputu: Artigo
Reo:Inglês
I whakaputaina: IOP Publishing 2024-01-01
Rangatū:The Astrophysical Journal Letters
Ngā marau:
Late-type supergiant stars
Stellar mass loss
Stellar radii
Long period variable stars
Yellow hypergiant stars
Hypergiant stars
Urunga tuihono:https://doi.org/10.3847/2041-8213/ad736c
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