Preliminary result of the analysis of T Sagittarrii data and modeling

Details Preliminary result of the analysis of T Sagittarrii data and modeling Preliminary result of the analysis of T Sagittarrii data and modeling

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004spie.5491.1733m&link_type=abstract

New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The Intern

Physics

1

Scientific paper

This document shows the first results of the study of the environment of
the S star T Sagittarii. Observational constraints are obtained through
10 μm long baseline interferometry with MIDI at the VLTI. Models of
the dust envelope are simulated with a monte-carlo radiative transfer
code.

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