2006/07/17 by T. Giannini, C. McCoey, B. Nisini +4 · 45 citations
Chemistry · Earth and Planetary Sciences · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Atmospheric Ozone and Climate #Emission spectrum #Far infrared #Infrared #Infrared spectroscopy #Line (geometry) #Molecular Spectroscopy and Structure #Near-infrared spectroscopy #Optics #Physics #Satellite #Spectral line #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065127
published in Astronomy and Astrophysics 459(3), 821-835 (EDP Sciences)
arxiv created 2006/07/17 · openalex publication_date 2006/08/31 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims.We present a detailed study of the infrared line emission (1–200 μm) in the Herbig-Haro object HH54. Our database comprises: high- (R ~ 9000) and low- (R ~ 600) resolution spectroscopic data in the near-infrared band (1–2.5 μm); mid-infrared spectrophotometric images (5–12 μm); and, far-IR (45–200 μm, R ~ 200) spectra acquired with the ISO satellite. As a result, we provide the detection of and the absolute fluxes for more than 60 molecular features (mainly from H2 in the near- and mid-infrared and from H2O, CO and OH in the far-infrared) and 23 ionic lines.