银河系中的质量组装与化学复杂性
星系天体物理
2025-12-17 v1
摘要
（亚）毫米光谱线不仅可用于理解我们星系中观测区域的化学复杂性与富集历史，而且通过光谱分辨的谱线，它们揭示了星系气体组分的物理条件、动力学，甚至电离状态与磁场强度。它们是跨尺度质量组装与结构形成的首要示踪剂。
引用
@article{arxiv.2512.14203,
title = {Mass Assembly and Chemical Complexity in the Milky Way},
author = {Pamela Klaassen and David Eden and Alessio Traficante and Henrik Beuther and Maite Beltrán and Caroline Bot and Elias Brinks and Laura Colzi and Timea Csengeri and Antoine Gusdorf and Doug Johnstone and Jes K. Jørgensen and Jonathan Marshall and Elena Redaelli and Víctor M. Rivilla and Thomas Stanke},
journal= {arXiv preprint arXiv:2512.14203},
year = {2025}
}
备注
This white paper was submitted to ESO Expanding Horizons in support of next generation sub-mm facilities