Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Facultad de Ciencias Exactas y Naturales de la UBA | - |
| dc.contributor | Curé, M. | - |
| dc.contributor | <div class="autor_fcen" id="7237">Rial, D.F.</div> | - |
| dc.contributor | Cidale, L. | - |
| dc.creator | Curé, M. | - |
| dc.creator | <div class="autor_fcen" id="7237">Rial, D.F.</div> | - |
| dc.creator | Cidale, L. | - |
| dc.date.accessioned | 2018-05-04T22:01:14Z | - |
| dc.date.accessioned | 2018-05-28T15:47:25Z | - |
| dc.date.available | 2018-05-04T22:01:14Z | - |
| dc.date.available | 2018-05-28T15:47:25Z | - |
| dc.date.issued | 2005 | - |
| dc.identifier.uri | http://10.0.0.11:8080/jspui/handle/bnmm/68293 | - |
| dc.description | The effects of rapid rotation and bi-stability upon the density contrast between the equatorial and polar directions of a B[e] supergiant are re-investigated. Based on a new slow solution for different high rotational radiation-driven winds and the fact that bi-stability allows a change in the line-force parameters (α, k, and δ), the equatorial densities are about 102-104 times higher than the polar ones. These values are in qualitative agreement with the observations. © ESO 2005. | - |
| dc.description | Fil:Rial, D.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | http://creativecommons.org/licenses/by/2.5/ar | - |
| dc.source | Astron. Astrophys. 2005;437(3):929-933 | - |
| dc.source.uri | http://digital.bl.fcen.uba.ar/Download/paper/paper_00046361_v437_n3_p929_Cure.pdf | - |
| dc.subject | Stars: early-type | - |
| dc.subject | Stars: mass-loss | - |
| dc.subject | Stars: rotation | - |
| dc.subject | Stars: winds, outflows | - |
| dc.subject | Bifurcation (mathematics) | - |
| dc.subject | Ionization | - |
| dc.subject | Mathematical models | - |
| dc.subject | Optical bistability | - |
| dc.subject | Parameter estimation | - |
| dc.subject | Radiation | - |
| dc.subject | Temperature measurement | - |
| dc.subject | Velocity measurement | - |
| dc.subject | Stars:early-type | - |
| dc.subject | Stars:mass-loss | - |
| dc.subject | Stars:rotation | - |
| dc.subject | Stars:winds, outflows | - |
| dc.subject | Astrophysics | - |
| dc.title | Outflowing disk formation in B[e] supergiants due to rotation and bi-stability in radiation driven winds | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:ar-repo/semantics/artículo | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| Aparece en las colecciones: | FCEN - Facultad de Ciencias Exactas y Naturales. UBA | |
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