BOAO PHOTOMETRIC SURVEY OF GALACTIC OPEN CLUSTERS. III. CZERNIK 24 AND CZERNIK 27 |
Kim Sang-Chul
(Korea Astronomy and Space Science Institute)
Park Hong-Soo (Astronomy Program, SEES, Seoul National University) Sohn Sang-Mo Tony (Korea Astronomy and Space Science Institute) Lee Myung-Gyoon (Astronomy Program, SEES, Seoul National University) Park Byeong-Gon (Korea Astronomy and Space Science Institute) Sung Hwan-Kyung (Department of Astronomy and Space Science, Sejong University) Ann Hong-Bae (Department of Earth Science, Pusan National University) Chun Moo-Young (Korea Astronomy and Space Science Institute) Kim Seung-Lee (Korea Astronomy and Space Science Institute) Jeon Young-Beom (Korea Astronomy and Space Science Institute) Yuk In-Soo (Korea Astronomy and Space Science Institute) Lee Sang- Hyun (Gimhae Astronomical Observatory) |
1 |
A Reference Guide to the IRAF/DAOPHOT Package
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2 |
On star formation and chemical evolution in the Galactic disk
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3 |
The age of the oldest open clusters
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DOI ScienceOn |
4 |
DAOPHOT: A computer program for crowded-field stellar photometry
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DOI |
5 |
Berkeley 29, the most distant old open cluster
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DOI ScienceOn |
6 |
Some revised observational constraints on the formation and evolution of the Galactic disk
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DOI |
7 |
UBV RI photometric standard stars in the magnitude range 11:5 < V < 16:0 around the celestial equator
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8 |
BOAO photometric survey of Galactic open clusters. III. Czernik 24 and Czernik 27, in Star Clusters
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9 |
Development of the Galactic disk: A search for the oldest open clusters
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DOI |
10 |
UBV I charge-coupled device photometry of two old open clusters NGC 1798 and NGC 2192
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DOI ScienceOn |
11 |
Catalogue of Open Cluster Data (Observatoire de Strassbourg, Centre de Donnees Stellaires)
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12 |
CCD photometry of distant open cluster. I. Berkeley 22, Berkeley 29 and Berkeley 54
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13 |
Evolutionary tracks and isochrones for low-and intermediate-mass stars: From 0.15 to 7 <TEX>$M_{\bigodot}$</TEX> and from Z = 0:0004 to 0.03
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DOI ScienceOn |
14 |
Abundance gradients and their evolution in the Milky Way disk
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15 |
The galactic system of old star clusters: The development of the galactic disk
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DOI |
16 |
New catalogue of optically visible open clusters and candidates
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DOI ScienceOn |
17 |
Physical parameters of the old open cluster Trumpler 5
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18 |
The old open clusters of the Milky Way
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DOI ScienceOn |
19 |
Open clusters as a record of the past
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DOI |
20 |
Metallicities of old open clusters
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DOI ScienceOn |
21 |
New open stars clusters
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22 |
The old open clusters of the Milky Way;The Globular Cluster-Galaxy Connection
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23 |
Red giants in old open clusters
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DOI |
24 |
On the Galactic disc age-metallicity relation
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DOI ScienceOn |
25 |
Metal abundances in extremely distant Galactic open clusters. I. Berkeley 29 and Saurer 1
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DOI ScienceOn |
26 |
On the Galactic disk metallicity distribution from open clusters. I. New catalogs and abundance gradient
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DOI ScienceOn |
27 |
Galactic metallicity gradients derived from a sample of OB stars
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DOI |
28 |
BOAO photometric survey of Galactic open clusters. I. Berkeley 14, Collinder 74, Biurakan 9, and NGC 2355
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29 |
Old open clusters as tracers of Galactic evolution, Astronomy and Space Science Library, Vol. 255;The Evolution of the Milky Way
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30 |
BOAO photometric survey of Galactic open clusters. II. Physical parameters of 12 open clusters
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DOI ScienceOn |