A possible solution for the lack of EHB binaries in globular clusters
- Author
- HAN, Z1
[1] National Astronomical Observatories / Yunnan Observatory, the Chinese Academy of Sciences, Kunming 650011, China - Source
Astronomy and astrophysics (Berlin. Print). 2008, Vol 484, Num 3 ; L31-L34 ; ref : 1/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- binaries: close globular clusters: general stars: horizontal-branch stars: subdwarfs
- Keyword (fr)
- Age Amas galactique Amas globulaire Amas stellaire Binaire serrée Etoile branche horizontale Formation stellaire Modèle Paramètre physique Population stellaire Sous naine Taux formation
- Keyword (en)
- Age Galactic cluster Globular clusters Star clusters Close binary stars Horizontal-branch stars Star formation Models Physical parameter Stellar population Subdwarf Formation rate
- Keyword (es)
- Edad Conglomerado galáctico Modelo Parámetro físico Población estelar Subenana Grado formación
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20396138
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
Access to the document
Install on your browser
DOI
10.1051/0004-6361:200809614 
https://dx.doi.org/10.1051/0004-6361:200809614
"O:13:\"PanistOpenUrl\":36:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000idc\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:27:\"10.1051\/0004-6361:200809614\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:9:\"\u0000*\u0000jtitle\";s:42:\"Astronomy and astrophysics (Berlin. Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Astron. astrophys. (Berl., Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"484\";s:8:\"\u0000*\u0000issue\";s:1:\"3\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:7:\"L31-L34\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6361\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:3:\"HAN\";s:10:\"\u0000*\u0000aufirst\";s:1:\"Z\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:0:{}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"AAEJAF\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:8:\"\u0000*\u0000place\";s:8:\"Les Ulis\";s:6:\"\u0000*\u0000pub\";s:12:\"EDP Sciences\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Panist access
"O:12:\"IstexOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:27:\"10.1051\/0004-6361:200809614\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:9:\"\u0000*\u0000jtitle\";s:42:\"Astronomy and astrophysics (Berlin. Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Astron. astrophys. (Berl., Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"484\";s:8:\"\u0000*\u0000issue\";s:1:\"3\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:7:\"L31-L34\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6361\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:3:\"HAN\";s:10:\"\u0000*\u0000aufirst\";s:1:\"Z\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:0:{}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"AAEJAF\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:8:\"\u0000*\u0000place\";s:8:\"Les Ulis\";s:6:\"\u0000*\u0000pub\";s:12:\"EDP Sciences\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Istex access
"O:16:\"UnpaywallOpenUrl\":35:{s:8:\"\u0000*\u0000email\";s:27:\"assistance-portail@inist.fr\";s:6:\"\u0000*\u0000fmt\";N;s:6:\"\u0000*\u0000doi\";s:27:\"10.1051\/0004-6361:200809614\";s:6:\"\u0000*\u0000pii\";N;s:7:\"\u0000*\u0000pmid\";N;s:9:\"\u0000*\u0000atitle\";N;s:9:\"\u0000*\u0000jtitle\";N;s:9:\"\u0000*\u0000stitle\";N;s:7:\"\u0000*\u0000date\";N;s:9:\"\u0000*\u0000volume\";N;s:8:\"\u0000*\u0000issue\";N;s:8:\"\u0000*\u0000spage\";N;s:8:\"\u0000*\u0000epage\";N;s:8:\"\u0000*\u0000pages\";N;s:7:\"\u0000*\u0000issn\";N;s:8:\"\u0000*\u0000eissn\";N;s:9:\"\u0000*\u0000aulast\";N;s:10:\"\u0000*\u0000aufirst\";N;s:9:\"\u0000*\u0000auinit\";N;s:10:\"\u0000*\u0000auinitm\";N;s:5:\"\u0000*\u0000au\";N;s:9:\"\u0000*\u0000aucorp\";N;s:7:\"\u0000*\u0000isbn\";N;s:8:\"\u0000*\u0000coden\";N;s:8:\"\u0000*\u0000genre\";N;s:7:\"\u0000*\u0000part\";N;s:9:\"\u0000*\u0000btitle\";N;s:8:\"\u0000*\u0000title\";N;s:8:\"\u0000*\u0000place\";N;s:6:\"\u0000*\u0000pub\";N;s:10:\"\u0000*\u0000edition\";N;s:9:\"\u0000*\u0000tpages\";N;s:9:\"\u0000*\u0000series\";N;s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";N;}"
Unpaywall access
"O:16:\"EuropePMCOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:27:\"10.1051\/0004-6361:200809614\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:9:\"\u0000*\u0000jtitle\";s:42:\"Astronomy and astrophysics (Berlin. Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Astron. astrophys. (Berl., Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"484\";s:8:\"\u0000*\u0000issue\";s:1:\"3\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:7:\"L31-L34\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6361\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:3:\"HAN\";s:10:\"\u0000*\u0000aufirst\";s:1:\"Z\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:0:{}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"AAEJAF\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:8:\"\u0000*\u0000place\";s:8:\"Les Ulis\";s:6:\"\u0000*\u0000pub\";s:12:\"EDP Sciences\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Europe PubMed Central access
"O:11:\"BaseOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:27:\"10.1051\/0004-6361:200809614\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:9:\"\u0000*\u0000jtitle\";s:42:\"Astronomy and astrophysics (Berlin. Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Astron. astrophys. (Berl., Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"484\";s:8:\"\u0000*\u0000issue\";s:1:\"3\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:7:\"L31-L34\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6361\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:3:\"HAN\";s:10:\"\u0000*\u0000aufirst\";s:1:\"Z\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:0:{}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"AAEJAF\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:8:\"\u0000*\u0000place\";s:8:\"Les Ulis\";s:6:\"\u0000*\u0000pub\";s:12:\"EDP Sciences\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Base Search access
"O:12:\"ArXivOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:27:\"10.1051\/0004-6361:200809614\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:9:\"\u0000*\u0000jtitle\";s:42:\"Astronomy and astrophysics (Berlin. Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Astron. astrophys. (Berl., Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2008\";s:9:\"\u0000*\u0000volume\";s:3:\"484\";s:8:\"\u0000*\u0000issue\";s:1:\"3\";s:8:\"\u0000*\u0000spage\";s:0:\"\";s:8:\"\u0000*\u0000epage\";s:0:\"\";s:8:\"\u0000*\u0000pages\";s:7:\"L31-L34\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-6361\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:3:\"HAN\";s:10:\"\u0000*\u0000aufirst\";s:1:\"Z\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:0:{}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"AAEJAF\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:69:\"A possible solution for the lack of EHB binaries in globular clusters\";s:8:\"\u0000*\u0000place\";s:8:\"Les Ulis\";s:6:\"\u0000*\u0000pub\";s:12:\"EDP Sciences\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
arXiv access
