Binary Lenses in OGLE-III EWS Database. Season 2004

dc.creatorJaroszynski, M.
dc.creatorSkowron, J.
dc.creatorUdalski, A.
dc.creatorKubiak, M.
dc.creatorSzymanski, M. K.
dc.creatorPietrzynski, G.
dc.creatorSoszynski, I.
dc.creatorZebrun, K.
dc.creatorSzewczyk, O.
dc.creatorWyrzykowski, L.
dc.date2007-01-31
dc.date.accessioned2026-07-07T12:45:08Z
dc.date.available2026-07-07T12:45:08Z
dc.descriptionWe present 19 binary lens candidates from OGLE-III Early Warning System database for the season of 2004. We have also found five events interpreted as single mass lensing of double sources. The candidates have been selected by visual light curves inspection. Examining the models of binary lenses of this and our previous studies (10 caustic crossing events of OGLE-II seasons 1997--1999 and 15 binary lens events of OGLE-III seasons 2002--2003) we find one case of extreme mass ratio binary (q ~ 0.005, a known planetary lens OGLE 2003-BLG-235/MOA 2003-BLG-53) and almost all other models with mass ratios in the range 0.1<q<1.0, which may indicate the division between planetary systems and binary stars.
dc.description27 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0701919
dc.identifierhttp://arxiv.org/abs/astro-ph/0701919
dc.identifierActa Astron.56:307,2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/220997
dc.subjectAstrophysics
dc.titleBinary Lenses in OGLE-III EWS Database. Season 2004
dc.typetext

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