| dc.contributor.author |
Falcón Veloz, Nelson Leonardo |
|
| dc.date.accessioned |
2015-06-25T14:59:57Z |
|
| dc.date.available |
2015-06-25T14:59:57Z |
|
| dc.date.issued |
2005-06 |
|
| dc.identifier.citation |
14th European Workshop on White Dwarfs, ASP Conference Series, Vol. 334 Proceedings of a meeting held at Kiel, July 19-23, 2004. Edited by D. Koester and S. Moehler. San Francisco: Astronomical Society of the Pacific, 2005, p.69 |
es_ES |
| dc.identifier.issn |
1-58381-190-7 |
|
| dc.identifier.uri |
http://hdl.handle.net/123456789/1761 |
|
| dc.description |
14th European Workshop on White Dwarfs ASP Conference Series, Vol. 334, 2005 |
es_ES |
| dc.description.abstract |
The standard white dwarf (WD) cooling theory is revised when the heat flux is propagate by thermal waves in degenerate material. Before the relaxation time, the luminosity function is dampening oscillation and the WD-age increase. |
es_ES |
| dc.language.iso |
es_ES |
es_ES |
| dc.publisher |
ASP Astronomical Society of the Pacific |
es_ES |
| dc.relation.ispartofseries |
Volumen 334, 2005; |
|
| dc.subject |
Dwarf cooling |
es_ES |
| dc.subject |
Thermal waves |
es_ES |
| dc.subject |
Degenerate material |
es_ES |
| dc.subject |
Luminosity function |
es_ES |
| dc.subject |
Dampening oscillation |
es_ES |
| dc.title |
White dwarf cooling by means of heat waves |
es_ES |
| dc.type |
Article |
es_ES |
