Surface phenomena in general relativistic stellar models: critical mass and stability
- Author
- HERRERA, L; JIMENEZ, J; ESCULPI, M
Univ. cent. Venezuela, dep. fisica, Caracas, Venezuela - Source
Physics letters. A. 1988, Vol 130, Num 4-5, pp 211-216, 6 p ; ref : 12 ref
- CODEN
- PYLAAG
- ISSN
- 0375-9601
- Scientific domain
- Crystallography; Condensed state physics; Physics; Plasma physics
- Publisher
- Elsevier Science, Amsterdam
- Publication country
- Netherlands
- Document type
- Article
- Language
- English
- 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
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19567603
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
10.1016/0375-9601(88)90596-8 
https://dx.doi.org/10.1016/0375-9601(88)90596-8
"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:28:\"10.1016\/0375-9601(88)90596-8\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:9:\"\u0000*\u0000jtitle\";s:18:\"Physics letters. A\";s:9:\"\u0000*\u0000stitle\";s:14:\"Phys. lett., A\";s:7:\"\u0000*\u0000date\";s:4:\"1988\";s:9:\"\u0000*\u0000volume\";s:3:\"130\";s:8:\"\u0000*\u0000issue\";s:3:\"4-5\";s:8:\"\u0000*\u0000spage\";s:3:\"211\";s:8:\"\u0000*\u0000epage\";s:3:\"216\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0375-9601\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HERRERA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"L\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:10:\"JIMENEZ, J\";i:1;s:10:\"ESCULPI, M\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"PYLAAG\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:8:\"\u0000*\u0000place\";s:9:\"Amsterdam\";s:6:\"\u0000*\u0000pub\";s:16:\"Elsevier Science\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"6\";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:28:\"10.1016\/0375-9601(88)90596-8\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:9:\"\u0000*\u0000jtitle\";s:18:\"Physics letters. A\";s:9:\"\u0000*\u0000stitle\";s:14:\"Phys. lett., A\";s:7:\"\u0000*\u0000date\";s:4:\"1988\";s:9:\"\u0000*\u0000volume\";s:3:\"130\";s:8:\"\u0000*\u0000issue\";s:3:\"4-5\";s:8:\"\u0000*\u0000spage\";s:3:\"211\";s:8:\"\u0000*\u0000epage\";s:3:\"216\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0375-9601\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HERRERA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"L\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:10:\"JIMENEZ, J\";i:1;s:10:\"ESCULPI, M\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"PYLAAG\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:8:\"\u0000*\u0000place\";s:9:\"Amsterdam\";s:6:\"\u0000*\u0000pub\";s:16:\"Elsevier Science\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"6\";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:28:\"10.1016\/0375-9601(88)90596-8\";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:28:\"10.1016\/0375-9601(88)90596-8\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:9:\"\u0000*\u0000jtitle\";s:18:\"Physics letters. A\";s:9:\"\u0000*\u0000stitle\";s:14:\"Phys. lett., A\";s:7:\"\u0000*\u0000date\";s:4:\"1988\";s:9:\"\u0000*\u0000volume\";s:3:\"130\";s:8:\"\u0000*\u0000issue\";s:3:\"4-5\";s:8:\"\u0000*\u0000spage\";s:3:\"211\";s:8:\"\u0000*\u0000epage\";s:3:\"216\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0375-9601\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HERRERA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"L\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:10:\"JIMENEZ, J\";i:1;s:10:\"ESCULPI, M\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"PYLAAG\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:8:\"\u0000*\u0000place\";s:9:\"Amsterdam\";s:6:\"\u0000*\u0000pub\";s:16:\"Elsevier Science\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"6\";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:28:\"10.1016\/0375-9601(88)90596-8\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:9:\"\u0000*\u0000jtitle\";s:18:\"Physics letters. A\";s:9:\"\u0000*\u0000stitle\";s:14:\"Phys. lett., A\";s:7:\"\u0000*\u0000date\";s:4:\"1988\";s:9:\"\u0000*\u0000volume\";s:3:\"130\";s:8:\"\u0000*\u0000issue\";s:3:\"4-5\";s:8:\"\u0000*\u0000spage\";s:3:\"211\";s:8:\"\u0000*\u0000epage\";s:3:\"216\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0375-9601\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HERRERA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"L\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:10:\"JIMENEZ, J\";i:1;s:10:\"ESCULPI, M\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"PYLAAG\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:8:\"\u0000*\u0000place\";s:9:\"Amsterdam\";s:6:\"\u0000*\u0000pub\";s:16:\"Elsevier Science\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"6\";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:28:\"10.1016\/0375-9601(88)90596-8\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:9:\"\u0000*\u0000jtitle\";s:18:\"Physics letters. A\";s:9:\"\u0000*\u0000stitle\";s:14:\"Phys. lett., A\";s:7:\"\u0000*\u0000date\";s:4:\"1988\";s:9:\"\u0000*\u0000volume\";s:3:\"130\";s:8:\"\u0000*\u0000issue\";s:3:\"4-5\";s:8:\"\u0000*\u0000spage\";s:3:\"211\";s:8:\"\u0000*\u0000epage\";s:3:\"216\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0375-9601\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:7:\"HERRERA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"L\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:2:{i:0;s:10:\"JIMENEZ, J\";i:1;s:10:\"ESCULPI, M\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"PYLAAG\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:85:\"Surface phenomena in general relativistic stellar models: critical mass and stability\";s:8:\"\u0000*\u0000place\";s:9:\"Amsterdam\";s:6:\"\u0000*\u0000pub\";s:16:\"Elsevier Science\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:1:\"6\";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
