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| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Facultad de Ciencias Exactas y Naturales de la UBA | - |
| dc.contributor | Curé, M. | - |
| dc.contributor | Cidale, L. | - |
| dc.contributor | <div class="autor_fcen" id="7237">Rial, D.F.</div> | - |
| dc.creator | Curé, M. | - |
| dc.creator | Cidale, L. | - |
| dc.creator | <div class="autor_fcen" id="7237">Rial, D.F.</div> | - |
| dc.date.accessioned | 2018-05-04T21:55:53Z | - |
| dc.date.accessioned | 2018-05-28T15:47:35Z | - |
| dc.date.available | 2018-05-04T21:55:53Z | - |
| dc.date.available | 2018-05-28T15:47:35Z | - |
| dc.date.issued | 2012 | - |
| dc.identifier.uri | http://10.0.0.11:8080/jspui/handle/bnmm/68323 | - |
| dc.description | We calculated the influence of the limb-darkened finite-disk correction factor in the theory of radiation-driven winds from massive stars. We solved the one-dimensional m-CAK hydrodynamical equation of rotating radiation-driven winds for all three known solutions, i.e., fast, Ω-slow, and δ-slow. We found that for the fast solution, the mass-loss rate is increased by a factor of 10%, while the terminal velocity is reduced about 10%, when compared with the solution using a finite-disk correction factor from a uniformly bright star. For the other two slow solutions, the changes are almost negligible. Although we found that the limb darkening has no effects on the wind-momentum-luminosity relationship, it would affect the calculation of synthetic line profiles and the derivation of accurate wind parameters. © 2012. The American Astronomical Society. All rights reserved. | - |
| 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 | Astrophys. J. 2012;757(2) | - |
| dc.source.uri | http://digital.bl.fcen.uba.ar/Download/paper/paper_0004637X_v757_n2_p_Cure.pdf | - |
| dc.subject | hydrodynamics | - |
| dc.subject | methods: analytical | - |
| dc.subject | stars: early-type | - |
| dc.subject | stars: mass-loss | - |
| dc.subject | stars: rotation | - |
| dc.subject | stars: winds, outflows | - |
| dc.title | Limb-darkened radiation-driven winds from massive stars | - |
| 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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