Fast molecular jet from L1157-mm

2014/11/27 by M. Tafalla, R. Bachiller, B. Lefloch +4 · 1 citation
Engineering · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Astrophysics and Star Formation Studies #Combustion and flame dynamics #Free molecular flow #Jet (fluid) #Molecular cloud #Molecular spectroscopy #Outflow #Protostar #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201425255

published as A&A 573, L2 (2015) · 6 pages, 8 figures. Accepted for publication in Astronomy & Astrophysics

openalex publication_date 2014/11/27 · arxiv created 2014/12/03 · arxiv updated 2014/12/24 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. L1157-mm powers a molecular outflow that is well-known for its shock-induced chemical activity in several hot-spots.

Citations

• Shells, jets, and internal working surfaces in the molecular outflow from IRAS 04166+2706

Cited by

• Nature of shocks revealed by SOFIA OI observations in the Cepheus E protostellar outflow

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