The circumstellar environment and evolutionary state of the supergiant B[e] star Wd1-9

2013/10/04 by J. S. Clark, B. W. Ritchie, I. Negueruela · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Blue supergiant #Giant star #Herbig Ae/Be star #O-type star #Red supergiant #Star (game theory) #Stars #Stellar evolution #Stellar, planetary, and galactic studies #Supergiant #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201321412

16 pages, 7 figures, accepted for publication in Astronomy and Astrophysics

openalex publication_date 2013/10/04 · arxiv created 2013/11/19 · arxiv updated 2015/06/17 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Historically, supergiant (sg)B[e] stars have been difficult to include in theoretical schemes for the evolution of massive OB stars.

Citations

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• Spectroscopic observations of the candidate sgB[e]/X-ray binary CI Camelopardalis
• Discovery of extended radio emission in the young cluster Wd1
• A VLT/FLAMES survey for massive binaries in Westerlund 1
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• On the massive stellar population of the super star cluster Westerlund 1

Cited by

• Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling

Related

• EWOCS-IV: 1Ms ACIS Chandra observation of the supergiant B[e] star Wd1-9
• The massive binary population of the starburst cluster Westerlund 1
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• A Census of B[e] Supergiants
• Radio observations of the massive stellar cluster Westerlund 1