Grown-up stars physics with MATISSE
Abstract
MATISSE represents a great opportunity to image the environment around massive and evolved stars. This will allow one to put constraints on the circumstellar structure, on the mass ejection of dust and its reorganization , and on the dust-nature and formation processes. MATISSE measurements will often be pivotal for the understanding of large multiwavelength datasets on the same targets collected through many high-angular resolution facilities at ESO like sub-millimeter interferometry (ALMA), near-infrared adaptive optics (NACO, SPHERE), interferometry (PIONIER, GRAVITY), spectroscopy (CRIRES), and mid-infrared imaging (VISIR). Among main sequence and evolved stars, several cases of interest have been identified that we describe in this paper.
Cite
@article{arxiv.1607.02393,
title = {Grown-up stars physics with MATISSE},
author = {Florentin Millour and J Hron and A Chiavassa and G Weigelt and A Soulain and Z Khorrami and A Meilland and N Nardetto and C Paladini and A Domiciano de Souza and G Niccolini and K. -H Hofmann and D Schertl and P Stee and P Bendjoya and F Thévenin and F Vakili and P Berio and T Lanz and A Matter and P Cruzalèbes and R Petrov and B Lopez},
journal= {arXiv preprint arXiv:1607.02393},
year = {2016}
}
Comments
SPIE, Jun 2016, Edimbourgh, France