2015/03/17 by Ruud Visser, Edwin A. Bergin, Jes K. Jorgensen +1 · 69 citations
Chemistry · Physics and Astronomy · #Accretion (finance) #Accretion disc #Astro and Planetary Science #Astrophysics and Star Formation Studies #Chemical composition #Circumstellar envelope #Envelope (radar) #Fullerene Chemistry and Applications #Protostar #Spectroscopy #TRACER #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201425365
published in Astronomy and Astrophysics 577, A102 (EDP Sciences) · Accepted by A&A; 12 pages, 7 figures
arxiv created 2015/03/17 · openalex publication_date 2015/03/25 · arxiv updated 2015/05/13 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims. Accretion rates in low-mass protostars can be highly variable in time. Each accretion burst is accompanied by a temporary increase in luminosity, heating up the circumstellar envelope and altering the chemical composition of the gas and dust. This paper aims to study such chemical effects and discusses the feasibility of using molecular spectroscopy as a tracer of episodic accretion rates and timescales.