The circumbinary disc around the J-type C-star IRAS 18006-3213

2007/03/12 by P. Deroo, H. Van Winckel, T. Verhoelst +5 · 2 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Circumbinary planet #Context (archaeology) #Geology #Paleontology #Physics #Star (game theory) #Stars #Stellar, planetary, and galactic studies #Type (biology) #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066516

11 pages, 11 figures, accepted for publication in A&A

arxiv created 2007/03/12 · openalex publication_date 2007/03/13 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05

Abstract

Context.In the generally accepted, but poorly documented model, silicate J-type C-stars are binary objects for which the silicate emission originates from a circumbinary or a circumcompanion disc.

Citations

• A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization
• Mid‐Infrared Spectroscopy of Carbon Stars in the Small Magellanic Cloud
• The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks
• CARBON STARS

Cited by

• Very Large Telescope Interferometer observations of the dust geometry around R Coronae Borealis stars★
• Integral field spectroscopy of planetary nebulae: mapping the line diagnostics and hydrogen-poor zones with VLT FLAMES