标题： 奥利维耶·舍尼厄关于大质量恒星的工作 显示英文标题

标题： Olivier Chesneau's work on massive stars

摘要： 奥利维耶·谢斯诺在他的职业生涯中，以出色的想法和大量工作挑战了观测恒星天体物理学的多个领域，从2000年关于天鹅座P的第一篇论文，到2014年关于V838 Mon的最后一篇论文。他一直使用所有所谓的高角分辨率技术，因为这有助于他的科学成果的实现，即详细研究恒星周围环境的内部结构，无论是小质量（AGB星），大质量（超巨星），还是爆炸性（新星）。我将在这里重点介绍他在大质量恒星方面的工作。 显示英文摘要

摘要： Olivier Chesneau challenged several fields of observational stellar astrophysics with bright ideas and an impressive amount of work to make them real in the span of his career, from his first paper on P Cygni in 2000, up to his last one on V838 Mon in 2014. He was using all the so-called high-angular resolution techniques since it helped his science to be made, namely study in details the inner structure of the environments around stars, be it small mass (AGBs), more massive (supergiant stars), or explosives (Novae). I will focus here on his work on massive stars.