Uncovering stellar atmospheres with gravitational microlensing telescopes
| dc.creator | Dominik, M. | |
| dc.date | 2003-12-08 | |
| dc.date.accessioned | 2026-07-07T02:11:29Z | |
| dc.date.available | 2026-07-07T02:11:29Z | |
| dc.description | 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. | |
| dc.description | 3 pages in LaTeX2e, 2 EPS-figures embedded, uses 'ws-procs975x65.cls' and 'rotating_pr.sty' (supplied). To appear in the Proceedings of the Xth Marcel Grossmann Meeting on General Relativity (Rio de Janeiro, Brasil, 20-26 July 2003), ed. S. Perez Bergliaffa, M. Novello & R. Ruffini (World Scientific, Singapore) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0312200 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0312200 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7107 | |
| dc.subject | Astrophysics | |
| dc.title | Uncovering stellar atmospheres with gravitational microlensing telescopes | |
| dc.type | text |