The winds of the most massive stars as viewed from long-baseline interferometry: model predictions

Details The winds of the most massive stars as viewed from long-baseline interferometry: model predictions The winds of the most massive stars as viewed from long-baseline interferometry: model predictions

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010rmxac..38...48g&link_type=abstract

The Interferometric View on Hot Stars (Eds. Th. Rivinius & M. Curé) Revista Mexicana de Astronomía y Astrofísica (Serie de Confe

Astronomy and Astrophysics

Astronomy

Stars: Mass Loss

Scientific paper

Long-baseline interferometry is one of the only techniques capable of providing milli-arcsecond spatial resolution observations which are needed to resolve the winds of massive stars. We present predictions of the interferometric observables of massive stars based on the non-LTE radiative transfer code CMFGEN and the Busche & Hillier (2005) code. We also show how dramatically different the monochromatic images of the most massive stars will look when they have a non-spherical wind.

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