Multi-component absorption lines in theHSTspectra of α Scorpii B

2007/07/16 by Robert A. Baade, D. Reimers · 4 citations
Physics and Astronomy · #Stellar, planetary, and galactic studies #Astrophysics and Star Formation Studies #Astronomy and Astrophysical Research

paper · pdf · doi:10.1051/0004-6361:20077308

openalex publication_date 2007/07/16 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Context.Extended atmospheres of late-type supergiants are of special interest with regard to the mass-loss process, the circumstellar physico-chemistry, and the evolution of stars.

Citations

• Mid‐Infrared Images of the Circumstellar Dust around α Scorpii

Cited by

• Imaging the outward motions of clumpy dust clouds around the red supergiant Antares with VLT/VISIR
• The Antares emission nebula and mass loss of \sf α Scorpii A
• Spectral variability of the α Sco AB binary system observed with IUE
• Antares [wikipedia]