RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904

From the BV images of the metal-poor globular cluster NGC 1904 obtained with the 2K CCD camera equipped on the BOAO 1.8m telescope, we construct (B - V, V) color-magnitude diagram of the cluster. The apparent V magnitudes of the RGB bump and tip have been measured from the luminosity function of the...

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Main Authors: J.W. Kim, Y. Choi, S. H. Chun, J. Jung, A. Kang, Y.-J. Sohn
Format: Article
Language:English
Published: The Korean Space Science Society 2006-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2006/v23n2/OJOOBS_2006_v23n2_97.pdf
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author J.W. Kim
Y. Choi
S. H. Chun
J. Jung
A. Kang
Y.-J. Sohn
author_facet J.W. Kim
Y. Choi
S. H. Chun
J. Jung
A. Kang
Y.-J. Sohn
author_sort J.W. Kim
collection DOAJ
description From the BV images of the metal-poor globular cluster NGC 1904 obtained with the 2K CCD camera equipped on the BOAO 1.8m telescope, we construct (B - V, V) color-magnitude diagram of the cluster. The apparent V magnitudes of the RGB bump and tip have been measured from the luminosity function of the iteratively selected RGB stars in NGC 1904. Theoretical absolute Mv magnitudes of the RGB bump and tip are estimated using the Yonsei-Yale isochrones. The distance modulus of NGC 1904 has been derived by comparing the observed apparent V magnitude with the estimated absolute Mv magnitude of the RGB bump and tip.
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spelling doaj.art-f90a00c6f01c43b8b9e5aafab49ab1162024-01-02T10:42:23ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092006-06-012329710410.5140/JASS.2006.23.2.097RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904J.W. Kim0Y. Choi1S. H. Chun2J. Jung3A. Kang4Y.-J. Sohn5Department of Astronomy, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy, Yonsei University, Seoul 120-749, KoreaFrom the BV images of the metal-poor globular cluster NGC 1904 obtained with the 2K CCD camera equipped on the BOAO 1.8m telescope, we construct (B - V, V) color-magnitude diagram of the cluster. The apparent V magnitudes of the RGB bump and tip have been measured from the luminosity function of the iteratively selected RGB stars in NGC 1904. Theoretical absolute Mv magnitudes of the RGB bump and tip are estimated using the Yonsei-Yale isochrones. The distance modulus of NGC 1904 has been derived by comparing the observed apparent V magnitude with the estimated absolute Mv magnitude of the RGB bump and tip.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2006/v23n2/OJOOBS_2006_v23n2_97.pdfRGB bumpRGB tipdistanceNGC 1904photometry
spellingShingle J.W. Kim
Y. Choi
S. H. Chun
J. Jung
A. Kang
Y.-J. Sohn
RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904
Journal of Astronomy and Space Sciences
RGB bump
RGB tip
distance
NGC 1904
photometry
title RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904
title_full RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904
title_fullStr RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904
title_full_unstemmed RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904
title_short RED GIANT BRANCH OF THE METAL POOR GLOBULAR CLUSTERS: II. BUMP, TIP, AND DISTANCE OF NGC 1904
title_sort red giant branch of the metal poor globular clusters ii bump tip and distance of ngc 1904
topic RGB bump
RGB tip
distance
NGC 1904
photometry
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2006/v23n2/OJOOBS_2006_v23n2_97.pdf
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