发表机构
ESO（欧洲南方天文台）
机构由 AI 辅助整理，请以论文原文为准。AI 中文总结
本文旨在提高ESO天文界对CTAO科学机遇的认识，强调ALMA毫米/亚毫米波能力与CTAO TeV观测结合可开辟新发现途径，协同作用涵盖更广泛的物理过程与观测联系。
AI 中文摘要
本文旨在提高 ESO 天文界对即将建成的切伦科夫望远镜阵列（CTAO）所提供的科学机遇的认识，重点介绍了将阿塔卡马大型毫米/亚毫米波阵列（ALMA）的毫米/亚毫米波能力与 CTAO 的甚高能（TeV）观测相结合，能够为科学发现开辟新途径的案例。许多天体物理源和环境在两种波段中均展现出可探测的辐射过程；然而，协同作用不仅限于共同的辐射机制，还涵盖连接毫米波、亚毫米波和 TeV 能量的更广泛的物理过程和观测联系。
英文摘要
This article aims to raise awareness within the ESO astronomical community of the scientific opportunities offered by the upcoming Cherenkov Telescope Array, CTAO, highlighting cases where combining millimetre/submillimetre capabilities of the Atacama Large Millimeter / submillimeter Array, ALMA with the CTAO's very high energy, TeV, observations enables new avenues for discovery. Many astrophysical sources and environments exhibit emission processes detectable in both regimes; however, the synergies extend beyond shared emission mechanisms and include broader physical processes and observational connections linking millimetre, submillimetre and TeV energies.
Commentspublished in ESO Messenger, vol 196 (2026)
Journal refThe Messenger Issue 196, 2026
