Molecular hydrogen in the circumstellar environments of Herbig Ae/Be stars probed by FUSE

2008/04/16 by C. Martin-Zaïdi, C. Martin-Zaidi, M. Deleuil +9 · 1 citation
Chemistry · Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Circumstellar disk #Fullerene Chemistry and Applications #Fuse (electrical) #Herbig Ae/Be star #Hydrogen #Hydrogen molecule #Molecule #Stars #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079325

23 pages (including on-line material), accepted for publication in A&A

openalex publication_date 2008/04/16 · arxiv created 2008/04/30 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Molecular hydrogen (H2) gas is the most abundant molecule in the circumstellar (CS) environments of young stars. It is thus a key element in our understanding of the evolution of pre-main sequence stars and their environments towards the main sequence.

Citations

• The size distribution of interstellar grains
• Are Giant Planets Forming around HR 4796A?
• STIS Coronagraphic Imaging of the Herbig Ae Star: HD 163296
• H2and CO Emission from Disks around T Tauri and Herbig Ae Pre–Main‐Sequence Stars and from Debris Disks around Young Stars: Warm and Cold Circumstellar Gas
• A Circumstellar Disk Around β Pictoris
• Stabilization of the disk around β Pictoris by extremely carbon-rich gas
• Millimeter Observations and Modeling of the AB Aurigae System
• Spatially Resolved Circumstellar Structure of Herbig Ae/Be Stars in the Near‐Infrared

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