An asymmetry detected in the disk of κ Canis Majoris with AMBER/VLTI

2006/11/17 by A. Meilland, Anthony Meilland, F. Millour +106 · 2 citations
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Asymmetry #Canis #Circumstellar disk #Classical mechanics #Geology #Kinematics #Physics #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065410

arxiv created 2006/11/17 · openalex publication_date 2006/12/05 · arxiv updated 2009/12/01 · openalex created_date 2019/06/27 · openalex updated_date 2026/08/05

Abstract

Aims.We study the geometry and kinematics of the circumstellar environment of the Be star κ CMa in the Brγ emission line and its nearby continuum.

Citations

• Effects of gravitational darkening on the determination of fundamentalparameters in fast-rotating B-type stars
• The spinning-top Be star Achernar from VLTI-VINCI
• The calibration of interferometric visibilities obtained with single-mode optical interferometers
• Direct constraint on the distance ofγ2Velorum from AMBER/VLTI observations
• First direct detection of a Keplerian rotating disk around the Be star α Arae using AMBER/VLTI

Cited by

• Resolving the dusty circumstellar environment of the A[e] supergiant HD 62623 with the VLTI/MIDI
• Classical Be stars