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Herschel–PACS observations of shocked gas associated with the jets of L1448 and L1157

2013/07/09 by G. Santangelo, B. Nisini, S. Antoniucci +7 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Excitation #Position (finance) #Protostar #Shock (circulatory) #Shock wave #Space observatory #Stellar, planetary, and galactic studies #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201321674

Accepted for publication in Astronomy and Astrophysics

arxiv created 2013/07/09 · openalex publication_date 2013/07/12 · arxiv updated 2015/06/16 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. In the framework of the Water In Star-forming regions with Herschel (WISH) key program, several H2O (Eu > 190 K), high-J CO, [Oi], and OH transitions are mapped with Herschel-PACS in two shock positions along two prototypical outflows around the low-luminosity sources L1448 and L1157. Previous Herschel-HIFI H2O observations (Eu = 53−249 K) are also used. The aim is to derive a complete picture of the excitation conditions at the selected shock positions.

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