Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry

To derive the metallicities of M3 and M5, we used the shape of red giant branch, horizontal branch magnitude, and red giant branch bump on the (V - I) - V color magnitude diagrams. [Fe/H] values ranging -1.46 -1.69 for M3, and -1.00 -1.49 for M5 are estimated. This result leads the morpholgies of re...

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Main Authors: Young-Jong Sohn, Hyun-Chul Lee
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2000-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v18n1_1.pdf
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spelling doaj-30307f9c772b47cfb91f23d90799d2b12020-11-25T00:30:34ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14092000-06-01171110Metallicities of Globular Clusters m3 and m5 from VI CCD PhotometryYoung-Jong Sohn0Hyun-Chul Lee1Center for Space Astrophysics, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy, Yonsei University, Seoul 120-749, KoreaTo derive the metallicities of M3 and M5, we used the shape of red giant branch, horizontal branch magnitude, and red giant branch bump on the (V - I) - V color magnitude diagrams. [Fe/H] values ranging -1.46 -1.69 for M3, and -1.00 -1.49 for M5 are estimated. This result leads the morpholgies of red giant and horizontal branches on the (V-I) - v color magnitude diagrams can be good indirect metallicity indicators of galactic globular clusters.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v18n1_1.pdfGLOBULAR CLUSTERS M3 AND M5
collection DOAJ
language English
format Article
sources DOAJ
author Young-Jong Sohn
Hyun-Chul Lee
spellingShingle Young-Jong Sohn
Hyun-Chul Lee
Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry
Journal of Astronomy and Space Sciences
GLOBULAR CLUSTERS M3 AND M5
author_facet Young-Jong Sohn
Hyun-Chul Lee
author_sort Young-Jong Sohn
title Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry
title_short Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry
title_full Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry
title_fullStr Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry
title_full_unstemmed Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry
title_sort metallicities of globular clusters m3 and m5 from vi ccd photometry
publisher Korean Space Science Society (KSSS)
series Journal of Astronomy and Space Sciences
issn 2093-5587
2093-1409
publishDate 2000-06-01
description To derive the metallicities of M3 and M5, we used the shape of red giant branch, horizontal branch magnitude, and red giant branch bump on the (V - I) - V color magnitude diagrams. [Fe/H] values ranging -1.46 -1.69 for M3, and -1.00 -1.49 for M5 are estimated. This result leads the morpholgies of red giant and horizontal branches on the (V-I) - v color magnitude diagrams can be good indirect metallicity indicators of galactic globular clusters.
topic GLOBULAR CLUSTERS M3 AND M5
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v18n1_1.pdf
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AT hyunchullee metallicitiesofglobularclustersm3andm5fromviccdphotometry
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