Binary Lenses in OGLE-III EWS Database. Seasons 2006-2008

Binary Lenses in OGLE-III EWS Database. Seasons 2006-2008

We present 27 binary lens candidates from OGLE-III Early Warning System database for the seasons 2006-2008. The candidates have been selected by visual light curves inspection. Our sample of binary lens events consists now of 78 stellar systems and 7 extrasolar planets of OGLE-III published elsewher...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Acta astronomica 2010-01, Vol.60 (3), p.197-231
Hauptverfasser: Jaroszynski, M, Skowron, J, Udalski, A, Kubiak, M, Szymanski, M K, Pietrzynski, G, Soszynski, I, Wyrzykowski, L, Ulaczyk, K, Poleski, R
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 231
container_issue 3
container_start_page 197
container_title Acta astronomica
container_volume 60
creator Jaroszynski, M
Skowron, J
Udalski, A
Kubiak, M
Szymanski, M K
Pietrzynski, G
Soszynski, I
Wyrzykowski, L
Ulaczyk, K
Poleski, R
description We present 27 binary lens candidates from OGLE-III Early Warning System database for the seasons 2006-2008. The candidates have been selected by visual light curves inspection. Our sample of binary lens events consists now of 78 stellar systems and 7 extrasolar planets of OGLE-III published elsewhere. Examining the distribution of stellar binaries we find that the number of systems per logarithmic mass ratio interval increases with mass ratio q, in contradiction with our previous findings. Stellar binaries belong to the region 0.03 < q < 1 and there is a gap between them and a separate population of planets.
format Article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_miscellaneous_899160725</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>899160725</sourcerecordid><originalsourceid>FETCH-LOGICAL-p187t-7767c5786c5697f2c9ec832607ecdfbd567f3d897f19c0a43f6ce8ed32de80463</originalsourceid><addsrcrecordid>eNotjLFOwzAURT2ARGn7D96YjBw7tp9HKKFEitShoI6Vaz9LQcEpfenA3xMJlnN1dKVzwxZSykoYpd0duyf6nNUrqBfMP_clXH54h4WQeF_4bts1om1b3hz2_CVM4RQIH_keA42FuJLSihmwYrc5DITr_12yj9fmffMmut223Tx14lyBm4Rz1kXjwEZjvcsqeoyglZUOY8qnZKzLOsF8VT7KUOtsIwImrRKCrK1esoe_7vkyfl-RpuNXTxGHIRQcr3QE76u5poz-BX8mP-E</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>899160725</pqid></control><display><type>article</type><title>Binary Lenses in OGLE-III EWS Database. Seasons 2006-2008</title><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>Jaroszynski, M ; Skowron, J ; Udalski, A ; Kubiak, M ; Szymanski, M K ; Pietrzynski, G ; Soszynski, I ; Wyrzykowski, L ; Ulaczyk, K ; Poleski, R</creator><creatorcontrib>Jaroszynski, M ; Skowron, J ; Udalski, A ; Kubiak, M ; Szymanski, M K ; Pietrzynski, G ; Soszynski, I ; Wyrzykowski, L ; Ulaczyk, K ; Poleski, R</creatorcontrib><description>We present 27 binary lens candidates from OGLE-III Early Warning System database for the seasons 2006-2008. The candidates have been selected by visual light curves inspection. Our sample of binary lens events consists now of 78 stellar systems and 7 extrasolar planets of OGLE-III published elsewhere. Examining the distribution of stellar binaries we find that the number of systems per logarithmic mass ratio interval increases with mass ratio q, in contradiction with our previous findings. Stellar binaries belong to the region 0.03 &lt; q &lt; 1 and there is a gap between them and a separate population of planets.</description><identifier>ISSN: 0001-5237</identifier><language>eng</language><ispartof>Acta astronomica, 2010-01, Vol.60 (3), p.197-231</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780</link.rule.ids></links><search><creatorcontrib>Jaroszynski, M</creatorcontrib><creatorcontrib>Skowron, J</creatorcontrib><creatorcontrib>Udalski, A</creatorcontrib><creatorcontrib>Kubiak, M</creatorcontrib><creatorcontrib>Szymanski, M K</creatorcontrib><creatorcontrib>Pietrzynski, G</creatorcontrib><creatorcontrib>Soszynski, I</creatorcontrib><creatorcontrib>Wyrzykowski, L</creatorcontrib><creatorcontrib>Ulaczyk, K</creatorcontrib><creatorcontrib>Poleski, R</creatorcontrib><title>Binary Lenses in OGLE-III EWS Database. Seasons 2006-2008</title><title>Acta astronomica</title><description>We present 27 binary lens candidates from OGLE-III Early Warning System database for the seasons 2006-2008. The candidates have been selected by visual light curves inspection. Our sample of binary lens events consists now of 78 stellar systems and 7 extrasolar planets of OGLE-III published elsewhere. Examining the distribution of stellar binaries we find that the number of systems per logarithmic mass ratio interval increases with mass ratio q, in contradiction with our previous findings. Stellar binaries belong to the region 0.03 &lt; q &lt; 1 and there is a gap between them and a separate population of planets.</description><issn>0001-5237</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNotjLFOwzAURT2ARGn7D96YjBw7tp9HKKFEitShoI6Vaz9LQcEpfenA3xMJlnN1dKVzwxZSykoYpd0duyf6nNUrqBfMP_clXH54h4WQeF_4bts1om1b3hz2_CVM4RQIH_keA42FuJLSihmwYrc5DITr_12yj9fmffMmut223Tx14lyBm4Rz1kXjwEZjvcsqeoyglZUOY8qnZKzLOsF8VT7KUOtsIwImrRKCrK1esoe_7vkyfl-RpuNXTxGHIRQcr3QE76u5poz-BX8mP-E</recordid><startdate>20100101</startdate><enddate>20100101</enddate><creator>Jaroszynski, M</creator><creator>Skowron, J</creator><creator>Udalski, A</creator><creator>Kubiak, M</creator><creator>Szymanski, M K</creator><creator>Pietrzynski, G</creator><creator>Soszynski, I</creator><creator>Wyrzykowski, L</creator><creator>Ulaczyk, K</creator><creator>Poleski, R</creator><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20100101</creationdate><title>Binary Lenses in OGLE-III EWS Database. Seasons 2006-2008</title><author>Jaroszynski, M ; Skowron, J ; Udalski, A ; Kubiak, M ; Szymanski, M K ; Pietrzynski, G ; Soszynski, I ; Wyrzykowski, L ; Ulaczyk, K ; Poleski, R</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p187t-7767c5786c5697f2c9ec832607ecdfbd567f3d897f19c0a43f6ce8ed32de80463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Jaroszynski, M</creatorcontrib><creatorcontrib>Skowron, J</creatorcontrib><creatorcontrib>Udalski, A</creatorcontrib><creatorcontrib>Kubiak, M</creatorcontrib><creatorcontrib>Szymanski, M K</creatorcontrib><creatorcontrib>Pietrzynski, G</creatorcontrib><creatorcontrib>Soszynski, I</creatorcontrib><creatorcontrib>Wyrzykowski, L</creatorcontrib><creatorcontrib>Ulaczyk, K</creatorcontrib><creatorcontrib>Poleski, R</creatorcontrib><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><jtitle>Acta astronomica</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Jaroszynski, M</au><au>Skowron, J</au><au>Udalski, A</au><au>Kubiak, M</au><au>Szymanski, M K</au><au>Pietrzynski, G</au><au>Soszynski, I</au><au>Wyrzykowski, L</au><au>Ulaczyk, K</au><au>Poleski, R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Binary Lenses in OGLE-III EWS Database. Seasons 2006-2008</atitle><jtitle>Acta astronomica</jtitle><date>2010-01-01</date><risdate>2010</risdate><volume>60</volume><issue>3</issue><spage>197</spage><epage>231</epage><pages>197-231</pages><issn>0001-5237</issn><abstract>We present 27 binary lens candidates from OGLE-III Early Warning System database for the seasons 2006-2008. The candidates have been selected by visual light curves inspection. Our sample of binary lens events consists now of 78 stellar systems and 7 extrasolar planets of OGLE-III published elsewhere. Examining the distribution of stellar binaries we find that the number of systems per logarithmic mass ratio interval increases with mass ratio q, in contradiction with our previous findings. Stellar binaries belong to the region 0.03 &lt; q &lt; 1 and there is a gap between them and a separate population of planets.</abstract><tpages>35</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0001-5237
ispartof Acta astronomica, 2010-01, Vol.60 (3), p.197-231
issn 0001-5237
language eng
recordid cdi_proquest_miscellaneous_899160725
source Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection
title Binary Lenses in OGLE-III EWS Database. Seasons 2006-2008
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-21T17%3A55%3A28IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Binary%20Lenses%20in%20OGLE-III%20EWS%20Database.%20Seasons%202006-2008&rft.jtitle=Acta%20astronomica&rft.au=Jaroszynski,%20M&rft.date=2010-01-01&rft.volume=60&rft.issue=3&rft.spage=197&rft.epage=231&rft.pages=197-231&rft.issn=0001-5237&rft_id=info:doi/&rft_dat=%3Cproquest%3E899160725%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=899160725&rft_id=info:pmid/&rfr_iscdi=true