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Astrophysical Journal, ISSN 0004-637X, 02/2013, Volume 764, Issue 1
We present the first set of a new generation of models of massive stars with a solar composition extending between 13 and 120 M {sub Sun }, computed with and... 
stars: massive | stars: interiors | stars: evolution | stars: rotation | supernovae: general | ROTATION | EXPLOSIVES | INSTABILITY | TRANSPORT THEORY | DUSTS | LIMITING VALUES | SUPERNOVAE | CARBON MONOXIDE | ANGULAR MOMENTUM | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | ADVECTION | BINDING ENERGY | STELLAR WINDS
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2017, Volume 836, Issue 1
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 02/2017, Volume 836, Issue 1, p. 79
Journal Article
Acta Herpetologica, ISSN 1827-9635, 2014, Volume 9, Issue 2, pp. 167 - 177
The Montpellier snake Malpolon monspessulanus is a wide-ranging species that inhabits Western and Eastern Europe, North Africa and Middle East. Four clades... 
Mediterranean | Geometric morphometrics | Malpolon | Psammophiinae | Taxonomy | Phylogeography | Nonparametric MANOVA | Variation partitioning
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 07/2018, Volume 237, Issue 1, p. 13
We present a new grid of presupernova models of massive stars extending in mass between 13 and 120 M-circle dot, covering four metallicities (i.e., [Fe/H] = 0,... 
stars: massive | stars: interiors | stars: evolution | stars: rotation | supernovae: general | WEAK INTERACTION RATES | RED SUPERGIANTS | S-PROCESS | CHEMICAL EVOLUTION | LIGHT CURVES | MAIN-SEQUENCE | VLT-FLAMES SURVEY | WOLF-RAYET STARS | STELLAR EVOLUTION | ASTRONOMY & ASTROPHYSICS | RATE TABLES
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 454, Issue 4, pp. 4250 - 4266
We quantify the role of Population (Pop) III core-collapse supernovae (SNe) as the first cosmic dust polluters. Starting from a homogeneous set of stellar... 
Galaxy: halo | Supernovae: general | Galaxies: evolution | ISM: clouds | Stars: low-mass | EJECTA | POOR STARS | galaxies: evolution | SUPERNOVA | supernovae: general | GRAINS | EVOLUTION | RADIATIVE ASSOCIATION | ASTRONOMY & ASTROPHYSICS | stars: low-mass | NUCLEOSYNTHESIS | NUCLEATION | NUMERICAL SIMULATIONS
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2013, Volume 764, Issue 1, pp. 1 - 36
We present the first set of a new generation of models of massive stars with a solar composition extending between 13 and 120 M sub([middot in circle]),... 
Networks | Metallicity | Binding energy | Evolution | Explosions | Combustion | Rotating | Composition effects | Massive stars
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 01/2013, Volume 764, Issue 1, p. 21
Journal Article
The Astrophysical Journal Supplement Series, ISSN 0067-0049, 03/2011, Volume 193, Issue 1, pp. 16 - jQuery1323920260161='48'
We investigate the effects of thermonuclear reaction rate variations on 26Al production in massive stars. The dominant production sites in such events were... 
gamma rays | nuclear reactions, nucleosynthesis, abundances | stars | stars: evolution | supernovae: general | Uncertainty | Monte Carlo methods | Reactions (nuclear) | Computer simulation | Mathematical models | Combustion | Nuclear physics | Massive stars | Physics - Solar and Stellar Astrophysics
Journal Article
亚太热带生物医学杂志:英文版, ISSN 2221-1691, 2016, Volume 6, Issue 6, pp. 516 - 519
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 06/2004, Volume 608, Issue 1 I, pp. 405 - 410
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2015, Volume 454, Issue 4, pp. 4250 - 4250
We quantify the role of Population (Pop) III core-collapse supernovae (SNe) as the first cosmic dust polluters. Starting from a homogeneous set of stellar... 
Galactic halos | Ejecta | Cosmic dust | Grains | Stars | Explosions | Carbon | Standards
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 12/2008, Volume 689, Issue 2, pp. 1031 - 1043
We present a comprehensive abundance analysis of 27 heavy elements in bright giant stars of the globular clusters M4 and M5 based on high-resolution, high... 
SELF-POLLUTION SCENARIO | S-PROCESS | METAL-POOR STARS | stars: abundances | BRANCH STARS | OMEGA-CENTAURI | NEUTRON-CAPTURE ELEMENTS | Galaxy: abundances | R-PROCESS-RICH | ASTRONOMY & ASTROPHYSICS | MAGNESIUM ISOTOPES | LABORATORY TRANSITION-PROBABILITIES | globular clusters: individual (M4, M5) | GALACTIC CHEMICAL EVOLUTION
Journal Article
Frontiers in Psychology, ISSN 1664-1078, 05/2018, Volume 9, Issue MAY, p. 699
Journal Article
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