The billion-year-old clusters of the Magellanic Clouds
Five clusters of the Magellanic Clouds in the age range of about one billion years have faint enough photometry to allow comparison with theoretical models. Semiempirical relationships are derived from various theoretical models that allow a determination of ages and chemical abundances for the clus...
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| Veröffentlicht in: | Astrophys. J.; (United States) 1982-05, Vol.256, p.447 |
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| container_title | Astrophys. J.; (United States) |
| container_volume | 256 |
| creator | Hodge, P. W. |
| description | Five clusters of the Magellanic Clouds in the age range of about one billion years have faint enough photometry to allow comparison with theoretical models. Semiempirical relationships are derived from various theoretical models that allow a determination of ages and chemical abundances for the clusters in question. Values for (Fe/H) ranging from -0.8 to -1.3 are found, and ages range from 0.7 to 1.1 billion years. |
| doi_str_mv | 10.1086/159921 |
| format | Article |
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Values for (Fe/H) ranging from -0.8 to -1.3 are found, and ages range from 0.7 to 1.1 billion years.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/159921</identifier><language>eng</language><publisher>United States</publisher><subject>640105 - Astrophysics & Cosmology- Galaxies ; ABUNDANCE ; AGE ESTIMATION ; CHEMICAL COMPOSITION ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; ELEMENTS ; GALAXIES ; HYDROGEN ; IRON ; MAGELLANIC CLOUDS ; METALS ; NONMETALS ; STAR CLUSTERS ; STAR EVOLUTION ; TRANSITION ELEMENTS</subject><ispartof>Astrophys. 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J.; (United States)</title><description>Five clusters of the Magellanic Clouds in the age range of about one billion years have faint enough photometry to allow comparison with theoretical models. Semiempirical relationships are derived from various theoretical models that allow a determination of ages and chemical abundances for the clusters in question. Values for (Fe/H) ranging from -0.8 to -1.3 are found, and ages range from 0.7 to 1.1 billion years.</description><subject>640105 - Astrophysics & Cosmology- Galaxies</subject><subject>ABUNDANCE</subject><subject>AGE ESTIMATION</subject><subject>CHEMICAL COMPOSITION</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>ELEMENTS</subject><subject>GALAXIES</subject><subject>HYDROGEN</subject><subject>IRON</subject><subject>MAGELLANIC CLOUDS</subject><subject>METALS</subject><subject>NONMETALS</subject><subject>STAR CLUSTERS</subject><subject>STAR EVOLUTION</subject><subject>TRANSITION ELEMENTS</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1982</creationdate><recordtype>article</recordtype><recordid>eNot0MtKxDAYBeAgCtZRn6G4cBf9kzRpspTiDUbcjOCupLk4kdhIklnM2ztDXR0OfJzFQeiawB0BKe4JV4qSE9QQziTuGO9PUQMAHRas_zxHF6V8HytVqkFis3XtFGIMacZ7pzNO0bYm7kp1ubTJt_UA3vSXi1HPwbRDTDtbLtGZ17G4q_9coY-nx83wgtfvz6_DwxobIqFiT4kAqielhSXWaekNs7YH1UvBPRVaAnDQDAQ13hPCNZN68p33B-ossBW6WXZTqWEsJlRntibNszN15EAZsP6AbhdkciolOz_-5vCj834kMB4vGZdL2B9PClH2</recordid><startdate>19820515</startdate><enddate>19820515</enddate><creator>Hodge, P. W.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19820515</creationdate><title>The billion-year-old clusters of the Magellanic Clouds</title><author>Hodge, P. W.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c180t-f21602ab9a6d1dea8fc3dd7097865f26a80050a3062cff115a38abf4ffa8fed03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1982</creationdate><topic>640105 - Astrophysics & Cosmology- Galaxies</topic><topic>ABUNDANCE</topic><topic>AGE ESTIMATION</topic><topic>CHEMICAL COMPOSITION</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>ELEMENTS</topic><topic>GALAXIES</topic><topic>HYDROGEN</topic><topic>IRON</topic><topic>MAGELLANIC CLOUDS</topic><topic>METALS</topic><topic>NONMETALS</topic><topic>STAR CLUSTERS</topic><topic>STAR EVOLUTION</topic><topic>TRANSITION ELEMENTS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hodge, P. W.</creatorcontrib><creatorcontrib>Astronomy Department, University of Washington, Seattle</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astrophys. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hodge, P. W.</au><aucorp>Astronomy Department, University of Washington, Seattle</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The billion-year-old clusters of the Magellanic Clouds</atitle><jtitle>Astrophys. J.; (United States)</jtitle><date>1982-05-15</date><risdate>1982</risdate><volume>256</volume><spage>447</spage><pages>447-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Five clusters of the Magellanic Clouds in the age range of about one billion years have faint enough photometry to allow comparison with theoretical models. Semiempirical relationships are derived from various theoretical models that allow a determination of ages and chemical abundances for the clusters in question. Values for (Fe/H) ranging from -0.8 to -1.3 are found, and ages range from 0.7 to 1.1 billion years.</abstract><cop>United States</cop><doi>10.1086/159921</doi></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-637X |
| ispartof | Astrophys. J.; (United States), 1982-05, Vol.256, p.447 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_159921 |
| source | Alma/SFX Local Collection |
| subjects | 640105 - Astrophysics & Cosmology- Galaxies ABUNDANCE AGE ESTIMATION CHEMICAL COMPOSITION CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ELEMENTS GALAXIES HYDROGEN IRON MAGELLANIC CLOUDS METALS NONMETALS STAR CLUSTERS STAR EVOLUTION TRANSITION ELEMENTS |
| title | The billion-year-old clusters of the Magellanic Clouds |
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