Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud

We present BV light curves of EROS 1010 which is located in the central bar of the Large Magellanic Cloud. The BV light curves including BR and I light curves observed by the EROS and OGLE projects, have been analyzed using the 2005 version of the Wilson & Devinney Differential Correction progra...

Full description

Bibliographic Details
Main Authors: Kyeong-Soo Hong, Young-Woon Kang
Format: Article
Language:English
Published: The Korean Space Science Society 2009-09-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2009/v26n3/OJOOBS_2009_v26n3_295.pdf
_version_ 1797368772477059072
author Kyeong-Soo Hong
Young-Woon Kang
author_facet Kyeong-Soo Hong
Young-Woon Kang
author_sort Kyeong-Soo Hong
collection DOAJ
description We present BV light curves of EROS 1010 which is located in the central bar of the Large Magellanic Cloud. The BV light curves including BR and I light curves observed by the EROS and OGLE projects, have been analyzed using the 2005 version of the Wilson & Devinney Differential Correction program for the photometric solutions. The absolute dimensions of EROS 1010 were calculated by adopting the distance modulus of the Large Magellanic Cloud, m-M = 18.m3 ~ 18.m5.
first_indexed 2024-03-08T17:37:33Z
format Article
id doaj.art-fa5677bb05594361b88532092acb5219
institution Directory Open Access Journal
issn 2093-5587
2093-1409
language English
last_indexed 2024-03-08T17:37:33Z
publishDate 2009-09-01
publisher The Korean Space Science Society
record_format Article
series Journal of Astronomy and Space Sciences
spelling doaj.art-fa5677bb05594361b88532092acb52192024-01-02T12:02:39ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092009-09-0126329530410.5140/JASS.2009.26.3.295Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic CloudKyeong-Soo Hong0Young-Woon Kang1Dept. of Astronomy and Space Science, and Astrophysical Research Center for the Structure and Evolution of the Cosmos (ARCSEC), Sejong University, Seoul 143-747, KoreaDept. of Astronomy and Space Science, and Astrophysical Research Center for the Structure and Evolution of the Cosmos (ARCSEC), Sejong University, Seoul 143-747, KoreaWe present BV light curves of EROS 1010 which is located in the central bar of the Large Magellanic Cloud. The BV light curves including BR and I light curves observed by the EROS and OGLE projects, have been analyzed using the 2005 version of the Wilson & Devinney Differential Correction program for the photometric solutions. The absolute dimensions of EROS 1010 were calculated by adopting the distance modulus of the Large Magellanic Cloud, m-M = 18.m3 ~ 18.m5.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2009/v26n3/OJOOBS_2009_v26n3_295.pdfeclipsing binariesLMCdata analysis
spellingShingle Kyeong-Soo Hong
Young-Woon Kang
Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud
Journal of Astronomy and Space Sciences
eclipsing binaries
LMC
data analysis
title Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud
title_full Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud
title_fullStr Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud
title_full_unstemmed Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud
title_short Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud
title_sort light curve analyses of the eclipsing binary eros 1010 in the large magellanic cloud
topic eclipsing binaries
LMC
data analysis
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2009/v26n3/OJOOBS_2009_v26n3_295.pdf
work_keys_str_mv AT kyeongsoohong lightcurveanalysesoftheeclipsingbinaryeros1010inthelargemagellaniccloud
AT youngwoonkang lightcurveanalysesoftheeclipsingbinaryeros1010inthelargemagellaniccloud