A multi-transition molecular line study of inward motions towards massive star-forming cores
Yan Sun, Yu Gao

TL;DR
This study uses multi-transition molecular line observations to detect inward motions in 29 massive star-forming cores, identifying six strong infall candidates and establishing HCO$^+$(1-0) as the best tracer for inward motions.
Contribution
It provides the first comprehensive multi-transition survey to identify inward motions and infall candidates in massive star-forming regions, highlighting HCO$^+$(1-0) as the most effective tracer.
Findings
Inward motions are prominent in HCO$^+$(1-0), CS(2-1), or HNC(1-0) lines.
HCO$^+$(1-0) shows the highest occurrence of asymmetric profiles.
Six strong infall candidates were identified with extended infall signatures.
Abstract
A multi-transition 3mm molecular line single-pointing and mapping survey was carried out towards 29 massive star-forming cores in order to search for the signature of inward motions. Up to seven different transitions, optically thick lines HCO(1-0), CS(2-1), HNC(1-0), HCN(1-0), CO(1-0) and optically thin lines CO(1-0), CO(1-0) were observed towards each source. The normalized velocity differences (V, V) between the peak velocities of optically thick lines and optically thin line CO(1-0) for each source were derived. Prominent inward motions are probably present in either HCO(1-0) or CS(2-1) or HNC(1-0) observations in most sources. Our observations show that there is a significant difference in the incidence of blue shifted line asymmetric line profiles between CS(2-1) and HCO(1-0). The HCO(1-0)…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
