Warm SiO gas in molecular bullets associated with protostellaroutflows

2006/10/02 by B. Nisini, C. Codella, T. Giannini +6 · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics #Astrophysics and Star Formation Studies #Atmospheric Ozone and Climate #Context (archaeology) #Geology #Meteorology #Outflow #Physics #Protostar #Star formation #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065621

11pages, 9 figures, A&A accepted

arxiv created 2006/10/02 · openalex publication_date 2006/10/11 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context.We present the first SiO multiline analysis (from J = 2–1 to J = 11–10) of the molecular bullets along the outflows of the Class 0 sources L1448-mm and L1157-mm, obtained through observations with IRAM and JCMT.

Citations

• A highly collimated, extremely highvelocity outflow in Taurus
• Tracing the Shock Precursors in the L1448-mm/IRS 3 Outflows
• SiO J = 5-4 in the HH 211 Protostellar Jet Imaged with the Submillimeter Array

Cited by

• BROAD N2H+EMISSION TOWARD THE PROTOSTELLAR SHOCK L1157-B1