VLTI monitoring of the dust formation event of the Nova V1280 Scorpii

2008/04/25 by O. Chesneau, Olivier Chesneau, Dipankar Banerjee +21 · 3 citations
Engineering · Physics and Astronomy · #Aeronautics #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Context (archaeology) #Engineering #Environmental science #Event (particle physics) #Geology #Interferometry #Nova (rocket) #Physics #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809485

arxiv created 2008/04/25 · openalex publication_date 2008/06/04 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. We present the first high spatial-resolution monitoring of the dust-forming nova V1280 Sco, performed with the Very Large Telescope Interferometer (VLTI).

Citations

• User Manual for DUSTY
• The size distribution of interstellar grains
• Modelling the Galactic interstellar extinction distribution in three dimensions
• A study of the expanding envelope of Nova V1974 Cyg 1992 basedon IUE high resolution spectroscopy

Cited by

• Five-year optical and near-infrared observations of the extremely slow nova V1280 Scorpii
• The distances of the Galactic novae
• Discovery of Metastable Helium Absorption Lines in V1280 Scorpii