Exploració per autor "Gil Pons, Pilar"
Ara es mostren els items 8-27 de 36
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MECÀNICA (Examen final, 1r quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2021-01-25)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen final, 1r quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2022-01-17)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen final, 2n quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2022-06-01)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen final, 2n quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2020-07-01)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen final, 2n quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2023-06-01)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen parcial, 1r quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2020-11-13)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen parcial, 1r quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2021-11-05)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen parcial, 1r quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2022-10-26)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen parcial, 2n quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2022-04-01)
Examen
Accés restringit a la comunitat UPC -
MECÀNICA (Examen parcial, 2n quadrimestre)
Gil Pons, Pilar (Universitat Politècnica de Catalunya, 2023-04-01)
Examen
Accés restringit a la comunitat UPC -
Monash Chemical Yields Project (Mon¿ey) - Element production in low- and intermediate-mass stars of metallicities Z = 0 to 0.04
Doherty, Carolyn L.; Lattanzio, John C.; Angelou, George; Campbell, Simon W; Church, Ross; Constantino, Thomas; Cristallo, Sergio; Gil Pons, Pilar; Karakas, Amanda; Lugaro, Maria; Stancliffe, Richard (Cambridge University Press, 2016)
Comunicació de congrés
Accés obertThe Mon¿ey project will provide a large and homogeneous set of stellar yields for the low- and intermediate- mass stars and has applications particularly to galactic chemical evolution modelling. We describe our detailed ... -
Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars
Gil Pons, Pilar; Doherty, Carolyn; Campbell, Simon W; Gutiérrez Cabello, Jordi (EDP Sciences, 2022-12-01)
Article
Accés obertStellar models and nucleosynthetic yields of primordial to extremely metal-poor (EMP) stars are crucial to interpret the surface abundances of the most metal-poor stars observed and, ultimately, to better understand the ... -
Nucleosynthetic yields of Z=1e-5 intermediate-mass stars
Gil Pons, Pilar; Doherty, Carolyn L.; Gutiérrez Cabello, Jordi; Campbell, Simon W; Siess, Lionel; Lattanzio, John C. (EDP Sciences, 2020-10-23)
Article
Accés obertAbridged: Observed abundances of extremely metal-poor (EMP) stars in the Halo hold clues for the understanding of the ancient universe. Interpreting these clues requires theoretical stellar models at the low-Z regime. We ... -
On the fate of extremely low metallicity stars
Gil Pons, Pilar; Gutiérrez Cabello, Jordi; García-Berro Montilla, Enrique; Althaus, Leandro Gabriel (2008)
Article
Accés obertWe have computed and analyzed the evolution of intermediate-mass stars of metallicity Z = 10−5 from the main sequence until the early stages of the TP-(S)AGB phase. In order to check the influence of mixing we have ... -
Primordial black holes capture by stars and induced collapse to low-mass stellar black holes
Oncins Marco, Gerard; Miralda Escudé, Jordi; Gutiérrez Cabello, Jordi; Gil Pons, Pilar (Oxford University Press, 2022-10-04)
Article
Accés obertPrimordial black holes in the asteroid-mass window, which might constitute all the dark matter, can be captured by stars when they traverse them at low enough velocity. After being placed on a bound orbit during star ... -
Primordial to extremely metal-poor AGB and Super-AGB stars: White dwarf or supernova progenitors?
Gil Pons, Pilar; Doherty, Carolyn L.; Gutiérrez Cabello, Jordi; Siess, Lionel; Wattana Campbell, Simon; Lau, Herbert B.; Lattanzio, John C. (2018-11-29)
Article
Accés obertGetting a better understanding of the evolution and nucleosynthetic yields of the most metal-poor stars ( Z ¿ 10 ¿5 ) is critical because they are part of the big picture of the history of the primitive universe. Yet many ... -
Production of short-lived radioactive nuclei in super asymptotic giant branch star
Doherty, Carolyn L.; Lugaro, M.; Lau, H.; Siess, Lionel; Lattanzio, John; Gil Pons, Pilar (2012-08-08)
Article
Accés obert -
Production of short-lived radioactive nuclei in Super Asymptotic Giant Branch stars
Doherty, Carolyn L.; Lugaro, M.; Lau, H. H. B.; Siess, Lionel; Lattanzio, John; Gil Pons, Pilar (2012)
Text en actes de congrés
Accés obert -
Super and massive AGB stars - III. nucleosynthesis in metal-poor and very metal-poor stars - Z = 0.001 and 0.0001
Doherty, Carolyn L.; Gil Pons, Pilar; Lau, Herbert B.; Lattanzio, John C.; Siess, Lionel; Campbell, Simon W (2014-05)
Article
Accés obertWe present a new grid of stellar models and nucleosynthetic yields for super-AGB stars with metallicities Z = 0.001 and 0.0001, applicable for use within galactic chemical evolution models. Contrary to more metal-rich stars ... -
Super asymptotic giant branch stars. I - Evolution code comparison
Doherty, Carolyn L.; Siess, Lionel; Lattanzio, John; Gil Pons, Pilar (2010-01-01)
Article
Accés restringit per política de l'editorialWe present an extensive set of detailed stellar models in the mass range 7.7–10.5M over the metallicity range Z = 10−5–0.02. These models were produced using the Monash University version of the Mount Stromlo Stellar ...