Uncovering Stellar Atmospheres with Gravitational Microlensing Telescopes

Details Uncovering Stellar Atmospheres with Gravitational Microlensing Telescopes Uncovering Stellar Atmospheres with Gravitational Microlensing Telescopes

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1630d&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

A strong differential magnification over the face of the source star passing the caustic created by a binary lens star allows to measure its radial intensity profile with an angular resolution of 20-60 nas from broad-band photometric observations for ~ 15 stars per year and to study its chemical composition from time-resolved high-resolution spectroscopy for ~ 2 stars per year.

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