Resolving the ionized wind of the post-red supergiant IRC +10 420 with VLTI/AMBER

2007/11/30 by W. J. de Wit, R. D. Oudmaijer, M. A. T. Groenewegen +3 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Atmospheric sciences #Environmental science #Gamma-ray bursts and supernovae #Ion #Ionization #Physics #Red supergiant #Scale (ratio) #Stars #Stellar, planetary, and galactic studies #Supergiant #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078773

Accepted for publication in A&A

arxiv created 2007/11/30 · openalex publication_date 2008/01/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.The paper investigates the milli-arcsecond scale structure of the present-day wind of the post-red supergiant IRC +10 420.

Citations

• Arcsecond-resolution ^\mathsf12CO mapping of the yellow hypergiants IRC +10420 and AFGL 2343
• De-biasing interferometric visibilities in VLTI-AMBER data of low SNR observations

Cited by

• A Red Supergiant Nebula at 25 μm: Arcsecond-Scale Mass-Loss Asymmetries of μ Cephei