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Discovery of Sulfur Oxides in the Ejecta of a B[e] Supergiant

B[e] supergiants represent a rare class of luminous, evolved massive stars surrounded by dusty circumstellar disks. Since their intense UV fields were long thought to sterilize their surroundings, molecular detections beyond carbon monoxide have remained elusive, leaving their chemical reservoirs la...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Cristobal Bordiu, J. Ricardo Rizzo, David Navarro-Almaida, Asunción Fuente, Filomena Bufano, Grazia Umana, Sara Loru, Alan C. Ruggeri, Carla Buemi, Francesco Cavallaro, Luciano Cerrigone, Adriano Ingallinera, Paolo Leto, Simone Riggi, Corrado Trigilio
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2026-01-01
Schriftenreihe:The Astrophysical Journal Letters
Schlagworte:
Massive stars
Early-type supergiant stars
Circumstellar disks
Molecular gas
Astrochemistry
Stellar mass loss
Online-Zugang:https://doi.org/10.3847/2041-8213/ae7b2b
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