29-30 June 2021
Massive stars: birth, rotation, and chemical evolution
News: All participants are welcome to join our Slack channel (#s16_massive_stars) for discussions during and after the symposium.Aims and scope
Massive stars are important drivers of galaxy evolution via their strong ionising radiation, momentum transfer, and chemical enrichment. In fact, some elements produced by massive stars are also crucial building blocks of planets and life. However, massive star formation and evolution are subject to fundamental uncertainties. This symposium is divided into three parts, each of which will highlight a specific phase in the life of a massive star.
In the first part, the focus will lie on massive young stellar objects (mYSOs). The goal of the sessions is to discuss mYSO evolution from the earliest phases in dense clouds up to their arrival on the zero age main sequence (ZAMS). This will include topics such as cloud collapse and dense core formation; disk formation, fragmentation and dissipation; accretion phenomena and mechanisms; Herbig Be stars; as well as multiplicity.
In the second and third parts, the main sequence and post-main sequence phases will be scrutinised, with focus on rotational mixing (or more broadly, chemical mixing), which drastically modifies evolutionary pathways. This directly impacts the evolutionary fate of massive stars and their end products, which include gravitational-wave progenitors such as neutron stars and black holes. Despite its significance, the mixing processes in massive stars are poorly known and remain calibrated within order-of-magnitude estimates in evolutionary models. Moreover, stellar winds and binarity can affect the surface abundances of stars, leading to further uncertainties when inferring internal chemical mixing processes.
In this symposium, we are bringing together an international group of experts from within and outside of Europe across all career stages. The focus is on combining recent constraints from the key research areas of photometry, spectroscopy, asteroseismology, and stellar evolution modelling, and bridge observations, theory and modelling efforts in this important area of stellar astrophysics. Ultimately, our goal is to improve evolutionary models and our understanding of massive star evolution from birth to death.
The 6 symposium blocks are distributed into a 2:3:1 format covering mYSOs, main sequence, and post-main sequence evolution. Additionally, 2 lunch blocks are dedicated to poster presentations / flash talks.
Updated on Mon Jun 28 14:40:08 CEST 2021
European Astronomical Society