Young stars in the old galactic cluster NGC 188?
First, the age of the oldest known galactic cluster, according to recently published determinations, is briefly discussed. The now definitely established membership of four W UMa type contact binaries in this cluster is difficult to understand if the age of these stars is that of the cluster. It app...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 1984-10, Vol.139 (2), p.477-480 |
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description | First, the age of the oldest known galactic cluster, according to recently published determinations, is briefly discussed. The now definitely established membership of four W UMa type contact binaries in this cluster is difficult to understand if the age of these stars is that of the cluster. It appears therefore that these binaries are much younger and that several episodes of star formation took place in NGC 188. This conclusion is reached after a new study of the mean density of the four contact binaries and a critical discussion of the chemical composition and the mixing length parameter. |
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The now definitely established membership of four W UMa type contact binaries in this cluster is difficult to understand if the age of these stars is that of the cluster. It appears therefore that these binaries are much younger and that several episodes of star formation took place in NGC 188. This conclusion is reached after a new study of the mean density of the four contact binaries and a critical discussion of the chemical composition and the mixing length parameter.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>CODEN: AAEJAF</identifier><language>eng</language><publisher>Les Ulis: EDP Sciences</publisher><subject>Astronomy ; Earth, ocean, space ; Exact sciences and technology ; Globular clusters in the milky way ; Stellar clusters and associations ; Stellar systems. Galactic and extragalactic objects and systems. The universe</subject><ispartof>Astronomy and astrophysics (Berlin), 1984-10, Vol.139 (2), p.477-480</ispartof><rights>1985 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>315,781,785</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=9163990$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Vant Veer, F</creatorcontrib><title>Young stars in the old galactic cluster NGC 188?</title><title>Astronomy and astrophysics (Berlin)</title><description>First, the age of the oldest known galactic cluster, according to recently published determinations, is briefly discussed. The now definitely established membership of four W UMa type contact binaries in this cluster is difficult to understand if the age of these stars is that of the cluster. It appears therefore that these binaries are much younger and that several episodes of star formation took place in NGC 188. This conclusion is reached after a new study of the mean density of the four contact binaries and a critical discussion of the chemical composition and the mixing length parameter.</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Globular clusters in the milky way</subject><subject>Stellar clusters and associations</subject><subject>Stellar systems. Galactic and extragalactic objects and systems. 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Galactic and extragalactic objects and systems. The universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Vant Veer, F</creatorcontrib><collection>Pascal-Francis</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Vant Veer, F</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Young stars in the old galactic cluster NGC 188?</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>1984-10-01</date><risdate>1984</risdate><volume>139</volume><issue>2</issue><spage>477</spage><epage>480</epage><pages>477-480</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><coden>AAEJAF</coden><abstract>First, the age of the oldest known galactic cluster, according to recently published determinations, is briefly discussed. The now definitely established membership of four W UMa type contact binaries in this cluster is difficult to understand if the age of these stars is that of the cluster. It appears therefore that these binaries are much younger and that several episodes of star formation took place in NGC 188. This conclusion is reached after a new study of the mean density of the four contact binaries and a critical discussion of the chemical composition and the mixing length parameter.</abstract><cop>Les Ulis</cop><pub>EDP Sciences</pub><tpages>4</tpages></addata></record> |
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source | EDP Sciences; EZB Electronic Journals Library |
subjects | Astronomy Earth, ocean, space Exact sciences and technology Globular clusters in the milky way Stellar clusters and associations Stellar systems. Galactic and extragalactic objects and systems. The universe |
title | Young stars in the old galactic cluster NGC 188? |
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