Zoom-In ON hIgh-mass Star forMation


Investigador responsável
M. S. Nanda Kumar

Theory of high-mass star formation predict specific features: formation of near-equal binary systems, radiation Rayleigh-Taylor instabilities, bloated photosphere. The goals of this project are to use the cutting edge facilities such as VLT, ALMA, JWST, and VLTI-GRAVITY to observationally zoom-in on the nearest targets to examine them at a few hundred AU scales and test/confront theoretical scenarios.

Instituição financiadora
Fundação para a Ciência e a Tecnologia

Início: 15 dezembro 2016
Fim: 14 dezembro 2021

Fundação para a Ciência e Tecnologia