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STELLAR EVOLUTION AND NUCLEOSYNTHESIS
(Ref. FQM-292)
26
mayo
2025
mayo 2025
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A. Moya-Bedon, J.C. Suárez Yanes, A. García Hernández and S. Martin-Ruiz,  "Hybrid gamma Doradus-delta Scuti Pulsators: New Insights into the Physics of the Oscillations from Kepler Observations",  The Astrophysical Journal, vol.713 , L192-L197, 2010
R.L. Gilliland-, T.M. Brown-, J. Christensen-Dalsgaard-, H. Kjeldsen-, C. Aerts-, J.C. Suárez Yanes and A. Et-,  "KEPLER ASTEROSEISMOLOGY PROGRAM: INTRODUCTION AND FIRST RESULTS",  Publications of the Astronomical Society of the Pacific, vol.122 , 131-143, 2010
A. Grigahcène, A. Moya-Bedon, J.C. Suárez Yanes, A. García Hernández and S. Martin-Ruiz,  "Kepler observations: Light shed on the hybrid gamma Dorados-Delta Scuti pulsation phenomenon",  Astronomische Nachrichten, vol.331 , 989-992, 2010
L. Galbany González "Measurements of the Rate of Type Ia Supernovae at Redshift z < 0.3 from the SDSS-II Supernova Survey.",  The Astrophysical Journal, vol.713 , 1026-, 2010
J.D. Fernandez Bayo, R. Cabezon , O.M. Zamora Sanchez, M.I. Dominguez Aguilera, D. Garcia-Senz , C.A. Abia Ladron De Guevara and O. Straniero,  "MERGING IN THE COMMON ENVELOPE AND THE ORIGIN OF THE EARLY R-TYPE STARS",  ASTRONOMY & ASTROPHYSICS, vol.522 , 1-18, 2010
L. Piersanti-, R. Cabezon-, O.M. Zamora-Sanchez, M.I. Dominguez Aguilera, D. Garcia-Senz-, C.A. Abia Ladron De Guevara and O. Straniero-,  "MERGING IN THE COMMON ENVELOPE AND THE ORIGIN OF THE EARLY R-TYPE STARS",  Astronomy & Astrophysics, vol.522 , 1-18, 2010
E. Bravo , M.I. Dominguez Aguilera, C. Badenes , J.D. Fernandez Bayo and O. Straniero,  "METALLICITY AS A SOURCE OF DISPERSION IN THE SNIA BOLOMETRIC LIGHT CURVE LUMINOSITY¿WIDTH RELATIONSHIP",  ASTROPHYSICAL JOURNAL, vol.711 , 66-70, 2010
E. Bravo-, M.I. Dominguez Aguilera, C. Badenes-, L. Piersanti- and O. Straniero-,  "METALLICITY AS A SOURCE OF DISPERSION IN THE SNIA BOLOMETRIC LIGHT CURVE LUMINOSITY¿WIDTH RELATIONSHIP",  The Astrophysical Journal, vol.711 , 66-70, 2010

Última actualización del SICA: 30/04/2025

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