Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars
- Author
- BENZ, W1 ; HILLS, J. G
[1] Los Alamos national lab., theoretical div., Los Alamos NM 87545, United States - Source
The Astrophysical journal. 1987, Vol 323, Num 2, pp 614-628 ; 1 ; ref : 24 ref
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Binaire Collision Dynamique stellaire Etoile séquence principale Hydrodynamique Méthode numérique Perte masse Simulation numérique
- Keyword (en)
- Binary star Collision Stellar dynamics Main sequence star Hydrodynamics Digital method Mass loss Digital simulation
- Keyword (es)
- Binario Colisión Dinámica estelar Estrella secuencia principal Hidrodinámica Método numérico Pérdida masa Simulación numérica
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A10 Fundamental astronomy / 001E03A10C Celestial mechanics (including n-body problems)
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 7592669
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
10.1086/165857 
https://dx.doi.org/10.1086/165857
"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:14:\"10.1086\/165857\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"1987\";s:9:\"\u0000*\u0000volume\";s:3:\"323\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"614\";s:8:\"\u0000*\u0000epage\";s:3:\"628\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:4:\"BENZ\";s:10:\"\u0000*\u0000aufirst\";s:1:\"W\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:11:\"HILLS, J. G\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";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:14:\"10.1086\/165857\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"1987\";s:9:\"\u0000*\u0000volume\";s:3:\"323\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"614\";s:8:\"\u0000*\u0000epage\";s:3:\"628\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:4:\"BENZ\";s:10:\"\u0000*\u0000aufirst\";s:1:\"W\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:11:\"HILLS, J. G\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";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:14:\"10.1086\/165857\";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:14:\"10.1086\/165857\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"1987\";s:9:\"\u0000*\u0000volume\";s:3:\"323\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"614\";s:8:\"\u0000*\u0000epage\";s:3:\"628\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:4:\"BENZ\";s:10:\"\u0000*\u0000aufirst\";s:1:\"W\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:11:\"HILLS, J. G\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";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:14:\"10.1086\/165857\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"1987\";s:9:\"\u0000*\u0000volume\";s:3:\"323\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"614\";s:8:\"\u0000*\u0000epage\";s:3:\"628\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:4:\"BENZ\";s:10:\"\u0000*\u0000aufirst\";s:1:\"W\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:11:\"HILLS, J. G\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";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:14:\"10.1086\/165857\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"1987\";s:9:\"\u0000*\u0000volume\";s:3:\"323\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"614\";s:8:\"\u0000*\u0000epage\";s:3:\"628\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:4:\"BENZ\";s:10:\"\u0000*\u0000aufirst\";s:1:\"W\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:1:{i:0;s:11:\"HILLS, J. G\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:101:\"Three-dimensional hydrodynamical simulations of stellar collisions. I: Equal-mass main-sequence stars\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";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
