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Observations et modélisations spectro-interférométriques longue base des étoiles et de leur environnement proche
[article]
2017
arXiv
pre-print
With the construction of the VLTI (Very Large Telescope Interferometer of the European Observatory ESO for the southern hemisphere) it is now possible to make observations with resolutions of the order of milli-arc-seconds, especially in IR with AMBER instrument (Astronomical Multi Beam Recombine). These new capabilities allow us to better constrain the stellar structures such as polar jets, equatorial disks and flattened photospheres of rotating stars. Thus the estimation of stellar
arXiv:1709.07334v1
fatcat:bvj6wuyjuzeqzflaztff46jzia