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| DOI | 10.1051/0004-6361:20078961 | ||||
| Año | 2008 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Conclusions. The geometric distance we derive is by far the most accurate to a Cepheid, and among the most accurate to any star. RS Pup appears both as somewhat neglected and particularly promising to investigate the mass-loss history of Cepheids. Thanks to its highly accurate distance, it is also bound to become an important luminosity fiducial for the long period part of the period-luminosity diagram.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Kervella, P. | Hombre |
Univ Paris Diderot - Francia
LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique - Francia |
| 2 | Merand, Antoine | Hombre |
Georgia State Univ - Estados Unidos
Georgia State University - Estados Unidos |
| 3 | Szabados, Laszlo | - |
Konkoly Observ Budapest - Hungría
Konkoly Observatory Hungarian Academy of Sciences - Hungría Konkoly Observatory - Hungría |
| 4 | Fouque, Pascal | Hombre |
Univ Toulouse 3 - Francia
Universite Paul Sabatier Toulouse III - Francia Observatoire Midi-Pyrénées - Francia |
| 5 | Bersier, D. | Hombre |
Liverpool John Moores Univ - Reino Unido
Liverpool John Moores University - Reino Unido |
| 6 | Ségransan, Damien | Hombre |
ESO - Chile
European Southern Observatory Santiago - Chile |
| 7 | Perrin, G. | - |
Univ Paris Diderot - Francia
|