Sensitive survey for13CO, CN, H2CO, and SO in the disks of T Tauri and Herbig Ae stars

2015/04/10 by L. Reboussin, S. Guilloteau, M. Simon +6 · 20 citations
Chemistry · Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Emission spectrum #Molecular Spectroscopy and Structure #Molecular cloud #Physics #Spectral line #Star formation #Stars #T Tauri star #Young stellar object #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201525705

published in Astronomy and Astrophysics 578, A31 (EDP Sciences) · 18 pages, 5 figures, accepted for publication in A&A

openalex publication_date 2015/04/10 · arxiv created 2015/04/17 · arxiv updated 2015/06/03 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We attempt to determine the molecular composition of disks around young low-mass stars in the ρ Oph region and to compare our results with a similar study performed in the Taurus-Auriga region.

Citations

• A dual-frequency sub-arcsecond study of proto-planetary disks at mm wavelengths: first evidence for radial variations of the dust properties
• Grain-surface reactions in molecular clouds: the effect of cosmic rays and quantum tunnelling
• VLBA determinations of the distances to nearby star-forming regions
• ISOCAM observations of the ρ Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster