Direct constraint on the distance ofγ2Velorum from AMBER/VLTI observations

2006/10/31 by F. Millour, R. G. Petrov, R. Petrov +125 · 3 citations
Mathematics · Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Binary number #Binary star #Constraint (computer-aided design) #Context (archaeology) #Geology #Geometry #Interferometry #Mathematics #Physics #Star (game theory) #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065408

arxiv created 2006/10/31 · openalex publication_date 2006/11/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Interferometry can provide spatially resolved observations of massive star binary systems and their colliding winds, which thus far have been studied mostly with spatially unresolved observations.

Citations

• The calibration of interferometric visibilities obtained with single-mode optical interferometers

Cited by

• An asymmetry detected in the disk of κ Canis Majoris with AMBER/VLTI
• Observation of Double Star by Long Baseline Interferometry
• A new-age determination for γ2 Velorum from binary stellar evolution models